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A neutron star is a type of stellar remnant that can result from the gravitational collapse of a massive star during a Type II, Type Ib or Type Ic supernova event. Neutron stars are the densest and tiniest stars known to exist in the universe; although having only the diameter of about 10 km (6 mi), they may have a mass of several times that of the Sun. Neutron stars probably appear white to the naked eye.
Neutron stars are the end points of stars whose mass after nuclear burning is greater than the Chandrasekhar limit for white dwarfs, but whose mass is not great enough to overcome the neutron degeneracy pressure to become black holes. Such stars are composed almost entirely of neutrons, which are subatomic particles without net electrical charge and with slightly larger mass than protons. Neutron stars are very hot and are supported against further collapse by quantum degeneracy pressure due to the phenomenon described by the Pauli exclusion principle. This principle states that no two neutrons (or any other fermionic particles) can occupy the same place and quantum state simultaneously.
The discovery of pulsars in 1967 suggested that neutron stars exist. Born in supernova explosions, these bodies are "only" ~12-13 kilometers by radius and spin around as rapidly as 642 times a second,[1] or approximately 38,500 revolutions per minute. A typical neutron star has a mass between ~1.4 and 3.2 solar masses with a surface temperature of ~6 x 105 Kelvin [2][3][4] (see Chandrasekhar limit).[5][a] In contrast, the Sun's radius is about 60,000 times that. Neutron stars have overall densities of 3.7×1017 to 5.9×1017 kg/m3 (2.6×1014 to 4.1×1014 times the density of the Sun),[b] which is comparable to the approximate density of an atomic nucleus of 3×1017 kg/m3.[6] The neutron star's density varies from below 1×109 kg/m3 in the crust - increasing with depth - to above 6×1017 or 8×1017 kg/m3 deeper inside (denser than an atomic nucleus).[7] This density is approximately equivalent to the mass of a Boeing 747 compressed to the size of a small grain of sand. A normal-sized matchbox containing neutron star material would have a mass of approximately 5 trillion tonnes.
In general, compact stars of less than 1.44 solar masses – the Chandrasekhar limit – are white dwarfs, and above 2 to 3 solar masses (the Tolman–Oppenheimer–Volkoff limit), a quark star might be created; however, this is uncertain. Gravitational collapse will usually occur on any compact star between 10 and 25 solar masses and produce a black hole.[8] Some neutron stars rotate very rapidly and emit beams of electromagnetic radiation as pulsars. Gamma-ray bursts may be produced from rapidly rotating, high-mass stars that collapse to form a neutron star, or from the merger of binary neutron stars. There are thought to be on the order of 108 neutron stars in the galaxy, but they can only be easily detected in certain instances, such as if they are a pulsar or part of a binary system. Non-rotating and non-accreting neutron stars are virtually undetectable; however, the Hubble Space Telescope has observed one thermally radiating neutron star, called RX J185635-3754.
Any star with an initial main-sequence mass of around 10 solar masses or above has the potential to become a neutron star. As the star evolves away from the main sequence, subsequent nuclear burning produces an iron-rich core. When all nuclear fuel in the core has been exhausted, the core must be supported by degeneracy pressure alone. Further deposits of material from shell burning cause the core to exceed the Chandrasekhar limit. Electron degeneracy pressure is overcome and the core collapses further, sending temperatures soaring to over 5 billion Kelvin. At these temperatures, photodisintegration (the breaking up of iron nuclei into alpha particles by high- energy gamma rays) occurs. As the temperature climbs even higher, electrons and protons combine to form neutrons, releasing a flood of neutrinos. When densities reach nuclear density of 4 x 1017 kilograms per cubic meter, neutron degeneracy pressure halts the contraction. The infalling outer atmosphere of the star is flung outwards, becoming a Type II or Type Ib supernova. The remnant left is a neutron star. If it has a mass greater than about 2-3 solar masses, it collapses further to become a black hole. Other neutron stars are formed within close binaries.
As the core of a massive star is compressed during a supernova, and collapses into a neutron star, it retains most of its angular momentum. Since it has only a tiny fraction of its parent's radius (and therefore its moment of inertia is sharply reduced), a neutron star is formed with very high rotation speed, and then gradually slows down. Neutron stars are known to have rotation periods from about 1.4 ms to 30 seconds. The neutron star's density also gives it very high surface gravity, up to 7×1012 m/s2 with typical values of a few ×1012 m/s2 (that is more than 1011 times of that of Earth). One measure of such immense gravity is the fact that neutron stars have an escape velocity of around 100,000 km/s, about a third of the speed of light. Matter falling onto the surface of a neutron star would be accelerated to tremendous speed by the star's gravity. The force of impact would likely destroy the object's component atoms, rendering all its matter identical, in most respects, to the rest of the star.[citation needed]
The surface of the neutron star is made of iron. In the presence of a strong magnetic field the atoms of iron polymerize. The polymers pack to form a lattice with density about ten thousand times that of terrestrial iron and strength a million times that of steel. It has excellent electrical conductivity along the direction of the magnetic field, but is a good insulator perpendicular to this direction. Immediately beneath this surface the neutron star is still solid, but its composition is changing. Larger nuclei, particularly rich in neutrons, are formed, and materials that on Earth would be radioactive are stable in this environment, such as nickel-62. With increasing depth, the density rises. When its density reaches 400 billion times that of water, the nuclei can get no larger and neutrons start 'dripping' out. As the density goes up further, the nuclei dissolve in a sea of neutrons. The neutron fluid is a superfluid – it has no viscosity and no resistance to flow or movement. Within a few kilometres of the surface the density has reached the density of the atomic nucleus. Up to this point the properties of matter are reasonably well understood, but beyond it understanding becomes increasingly sketchy. The composition of the core of the star is particularly uncertain: it may be liquid or solid; it may consist of other nuclear particles (pions, for example, or hyperons); and there may be another phase change, where quarks start 'dripping' out of the neutrons, forming another liquid.
A neutron star has a mass comparable to that of the Sun, but as it is only about 10 km (6 mi) in radius, it has an average density 1 quadrillion times that of water. Such a large mass in such a small volume produces an intense gravitational force: objects weigh 100 billion times more on the surface of a neutron star than on the surface of the Earth. The intense gravitational field affects light and other electromagnetic radiation emitted by the star, producing significant redshift (z approximately equal to 0.2). The strong gravitational attraction allows neutron stars to spin rapidly (hundreds of revolutions per second) without disintegrating. Such spin rates are expected if the core of the original star collapses without loss of angular momentum - if the original star has a magnetic field, then this too may be conserved and concentrated in the collapse to a neutron star. Pulsars, gamma-ray burst sources, and the neutron stars in some X-ray binaries are believed to have magnetic fields with a strength of about 100 million Tesla (roughly a million million times the strength of the Earth's magnetic field).
The gravitational field at the star's surface is about 2×1011 times stronger than on Earth. Such a strong gravitational field acts as a gravitational lens and bends the radiation emitted by the star such that parts of the normally invisible rear surface become visible.[9]
A fraction of the mass of a star that collapses to form a neutron star is released in the supernova explosion from which it forms (from the law of mass-energy equivalence, E = mc2). The energy comes from the gravitational binding energy of a neutron star.
Neutron star relativistic equations of state provided by Jim Lattimer include a graph of radius vs. mass for various models.[10] The most likely radii for a given neutron star mass are bracketed by models AP4 (smallest radius) and MS2 (largest radius). BE is the ratio of gravitational binding energy mass equivalent to observed neutron star gravitational mass of "M" kilograms with radius "R" meters,[11]
Given current values
and star masses "M" commonly reported as multiples of one solar mass,
then the relativistic fractional binding energy of a neutron star is
A two-solar-mass neutron star would not be more compact than 10,970 meters radius (AP4 model). Its mass fraction gravitational binding energy would then be 0.187, −18.7% (exothermic). This is not near 0.6/2 = 0.3, −30%.
A neutron star is so dense that one teaspoon (5 milliliters) of its material would have a mass over 5.5×1012 kg (that is 1100 tonnes per 1 nanolitre), about 900 times the mass of the Great Pyramid of Giza.[c] Hence, the gravitational force of a typical neutron star is such that if an object were to fall from a height of one meter, it would only take one microsecond to hit the surface of the neutron star, and would do so at around 2000 kilometers per second, or 7.2 million kilometers per hour.[13]
The temperature inside a newly formed neutron star is from around 1011 to 1012 kelvin.[7] However, the huge number of neutrinos it emits carry away so much energy that the temperature falls within a few years to around 106 kelvin.[7] Even at 1 million kelvin, most of the light generated by a neutron star is in X-rays. In visible light, neutron stars probably radiate approximately the same energy in all parts of visible spectrum, and therefore appear white.
The pressure increases from 3×1033 to 1.6×1035 Pa from the inner crust to the center.[14]
The equation of state for a neutron star is still not known. It is assumed that it differs significantly from that of a white dwarf, whose EOS is that of a degenerate gas which can be described in close agreement with special relativity. However, with a neutron star the increased effects of general relativity can no longer be ignored. Several EOS have been proposed (FPS, UU, APR, L, SLy, and others) and current research is still attempting to constrain the theories to make predictions of neutron star matter.[5][15] This means that the relation between density and mass is not fully known, and this causes uncertainties in radius estimates. For example, a 1.5 solar mass neutron star could have a radius of 10.7, 11.1, 12.1 or 15.1 kilometres (for EOS FPS, UU, APR or L respectively).[15]
Current understanding of the structure of neutron stars is defined by existing mathematical models, but it might be possible to infer through studies of neutron-star oscillations. Similar to asteroseismology for ordinary stars, the inner structure might be derived by analyzing observed frequency spectra of stellar oscillations.[5]
On the basis of current models, the matter at the surface of a neutron star is composed of ordinary atomic nuclei crushed into a solid lattice with a sea of electrons flowing through the gaps between them. It is possible that the nuclei at the surface are iron, due to iron's high binding energy per nucleon.[16] It is also possible that heavy element cores, such as iron, simply sink beneath the surface, leaving only light nuclei like helium and hydrogen cores.[16] If the surface temperature exceeds 106 kelvin (as in the case of a young pulsar), the surface should be fluid instead of the solid phase observed in cooler neutron stars (temperature <106 kelvin).[16]
The "atmosphere" of the star is hypothesized to be at most several micrometers thick, and its dynamic is fully controlled by the star's magnetic field. Below the atmosphere one encounters a solid "crust". This crust is extremely hard and very smooth (with maximum surface irregularities of ~5 mm), because of the extreme gravitational field.[17]
Proceeding inward, one encounters nuclei with ever increasing numbers of neutrons; such nuclei would decay quickly on Earth, but are kept stable by tremendous pressures. As this process continues at increasing depths, neutron drip becomes overwhelming, and the concentration of free neutrons increases rapidly. In this region, there are nuclei, free electrons, and free neutrons. The nuclei become increasingly small (gravity and pressure overwhelming the strong force) until the core is reached, by definition the point where they disappear altogether.
The composition of the superdense matter in the core remains uncertain. One model describes the core as superfluid neutron-degenerate matter (mostly neutrons, with some protons and electrons). More exotic forms of matter are possible, including degenerate strange matter (containing strange quarks in addition to up and down quarks), matter containing high-energy pions and kaons in addition to neutrons,[5] or ultra-dense quark-degenerate matter.
In 1934, Walter Baade and Fritz Zwicky proposed the existence of the neutron star,[18][d] only a year after the discovery of the neutron by Sir James Chadwick.[21] In seeking an explanation for the origin of a supernova, they tentatively proposed that in supernova explosions ordinary stars are turned into stars that consist of extremely closely packed neutrons that they called neutron stars. Baade and Zwicky correctly proposed at that time that the release of the gravitational binding energy of the neutron stars powers the supernova: "In the supernova process, mass in bulk is annihilated". Neutron stars were thought to be too faint to be detectable and little work was done on them until November 1967, when Franco Pacini (1939– ) pointed out that if the neutron stars were spinning and had large magnetic fields, then electromagnetic waves would be emitted. Unbeknown to him, radio astronomer Antony Hewish and his research assistant Jocelyn Bell at Cambridge were shortly to detect radio pulses from stars that are now believed to be highly magnetized, rapidly spinning neutron stars, known as pulsars.
In 1965, Antony Hewish and Samuel Okoye discovered "an unusual source of high radio brightness temperature in the Crab Nebula".[22] This source turned out to be the Crab Nebula neutron star that resulted from the great supernova of 1054.
In 1967, Iosif Shklovsky examined the X-ray and optical observations of Scorpius X-1 and correctly concluded that the radiation comes from a neutron star at the stage of accretion.[23]
In 1967, Jocelyn Bell and Antony Hewish discovered regular radio pulses from CP 1919. This pulsar was later interpreted as an isolated, rotating neutron star. The energy source of the pulsar is the rotational energy of the neutron star. The majority of known neutron stars (about 2000, as of 2010) have been discovered as pulsars, emitting regular radio pulses.
In 1971, Riccardo Giacconi, Herbert Gursky, Ed Kellogg, R. Levinson, E. Schreier, and H. Tananbaum discovered 4.8 second pulsations in an X-ray source in the constellation Centaurus, Cen X-3. They interpreted this as resulting from a rotating hot neutron star. The energy source is gravitational and results from a rain of gas falling onto the surface of the neutron star from a companion star or the interstellar medium.
In 1974, Antony Hewish was awarded the Nobel Prize in Physics "for his decisive role in the discovery of pulsars" without Jocelyn Bell who shared in the discovery.
In 1974, Joseph Taylor and Russell Hulse discovered the first binary pulsar, PSR B1913+16, which consists of two neutron stars (one seen as a pulsar) orbiting around their center of mass. Einstein's general theory of relativity predicts that massive objects in short binary orbits should emit gravitational waves, and thus that their orbit should decay with time. This was indeed observed, precisely as general relativity predicts, and in 1993, Taylor and Hulse were awarded the Nobel Prize in Physics for this discovery.
In 1982, Don Backer and colleagues discovered the first millisecond pulsar, PSR B1937+21. This objects spins 642 times per second, a value that placed fundamental constraints on the mass and radius of neutron stars. Many millisecond pulsars were later discovered, but PSR B1937+12 remained the fastest-spinning known pulsar for 24 years, until PSR J1748-2446ad was discovered.
In 2003, Marta Burgay and colleagues discovered the first double neutron star system where both components are detectable as pulsars, PSR J0737-3039. The discovery of this system allows a total of 5 different tests of general relativity, some of these with unprecedented precision.
In 2010, Paul Demorest and colleagues measured the mass of the millisecond pulsar PSR J1614–2230 to be 1.97±0.04 solar masses, using Shapiro delay.[24] This was substantially higher than any previously measured neutron star mass (1.67 solar masses, see PSR J1903+0327), and places strong constraints on the interior composition of neutron stars.
In 2013, John Antoniadis and colleagues measured the mass of PSR J0348+0432 to be 2.01±0.04 solar masses, using white dwarf spectroscopy .[25] This confirmed the existence of such massive stars using a different method. Furthermore, this allowed, for the first time, a test of general relativity using such a massive neutron star.
Neutron stars rotate extremely rapidly after their creation due to the conservation of angular momentum; like spinning ice skaters pulling in their arms, the slow rotation of the original star's core speeds up as it shrinks. A newborn neutron star can rotate several times a second; sometimes, the neutron star absorbs orbiting matter from a companion star, increasing the rotation to several hundred times per second, reshaping the neutron star into an oblate spheroid.
Over time, neutron stars slow down (spin down) because their rotating magnetic fields radiate energy; older neutron stars may take several seconds for each revolution.
The rate at which a neutron star slows its rotation is usually constant and very small: the observed rates of decline are between 10−10 and 10−21 seconds for each rotation. Therefore, for a typical slow down rate of 10−15 seconds per rotation, a neutron star now rotating in 1 second will rotate in 1.000003 seconds after a century, or 1.03 seconds after 1 million years.
Sometimes a neutron star will spin up or undergo a glitch, a sudden small increase of its rotation speed. Glitches are thought to be the effect of a starquake — as the rotation of the star slows down, the shape becomes more spherical. Due to the stiffness of the "neutron" crust, this happens as discrete events when the crust ruptures, similar to tectonic earthquakes. After the starquake, the star will have a smaller equatorial radius, and since angular momentum is conserved, rotational speed increases. Recent work, however, suggests that a starquake would not release sufficient energy for a neutron star glitch; it has been suggested that glitches may instead be caused by transitions of vortices in the superfluid core of the star from one metastable energy state to a lower one.[26]
Neutron stars have been observed to "pulse" radio and x-ray emissions believed to be caused by particle acceleration near the magnetic poles, which need not be aligned with the rotation axis of the star. Through mechanisms not yet entirely understood, these particles produce coherent beams of radio emission. External viewers see these beams as pulses of radiation whenever the magnetic pole sweeps past the line of sight. The pulses come at the same rate as the rotation of the neutron star, and thus, appear periodic. Neutron stars which emit such pulses are called pulsars.
The most rapidly rotating neutron star currently known, PSR J1748-2446ad, rotates at 716 rotations per second.[27] A recent paper reported the detection of an X-ray burst oscillation (an indirect measure of spin) at 1122 Hz from the neutron star XTE J1739-285.[28] However, at present, this signal has only been seen once, and should be regarded as tentative until confirmed in another burst from this star.
At present, there are about 2000 known neutron stars in the Milky Way and the Magellanic Clouds, the majority of which have been detected as radio pulsars. Neutron stars are most concentrated along the disk of the Milky Way although the spread perpendicular to the disk is large because the supernova explosion process can impart high speeds (400 km/s) to the newly created neutron star.
Some of the closest neutron stars are RX J1856.5-3754 about 400 light years away and PSR J0108-1431 at about 424 light years.[29] Another nearby neutron star that was detected transiting the backdrop of the constellation Ursa Minor has been catalogued as 1RXS J141256.0+792204. This rapidly moving object, nicknamed "Calvera" by its Canadian and American discoverers, was discovered using the ROSAT/Bright Source Catalog. Initial measurements placed its distance from Earth at 200 to 1,000 light years away, with later claims at about 450 light-years.
About 5% of all known neutron stars are members of a binary system. The formation and evolution scenario of binary neutron stars is a rather exotic and complicated process.[30] The companion stars may be either ordinary stars, white dwarfs or other neutron stars. According to modern theories of binary evolution it is expected that neutron stars also exist in binary systems with black hole companions. Such binaries are expected to be prime sources for emitting gravitational waves. Neutron stars in binary systems often emit X-rays which is caused by the heating of material (gas) accreted from the companion star. Material from the outer layers of a (bloated) companion star is sucked towards the neutron star as a result of its very strong gravitational field. As a result of this process binary neutron stars may also coalesce into black holes if the accretion of mass takes place under extreme conditions.[31] It has been proposed that coalescence of binaries consisting of two neutron stars may be responsible for producing short gamma-ray bursts. Such events may also be responsible for creating all chemical elements beyond iron,[32] as opposed to the supernova nucleosynthesis theory.
A neutron star has some of the properties of an atomic nucleus, including density and being composed of nucleons. In popular scientific writing, neutron stars are therefore sometimes described as giant nuclei. However, in other respects, neutron stars and atomic nuclei are quite different. In particular, a nucleus is held together by the strong interaction, whereas a neutron star is held together by gravity. It is generally more useful to consider such objects as stars.
|Wikimedia Commons has media related to Neutron stars.


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Missing Numbers: At the Pond
Freddy the Frog is on a mission to find missing lily pads and get his pond back to the way he likes it. By writing the missing numbers – all even – on the empty spaces in the lily pad grid, kids can practice counting whole numbers to 100, counting by twos, identifying even numbers and number writing.
Topics: First Grade, Counting
Updated on Jan 28, 2014
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1 January, 2000@12:00 am
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Take notice of a common trend in hip-hop music. Every year, a "new" artist or producer gets enough of a buzz surrounding them, that every label is asking them to hop on a remix or guest appear on some other artist's record. Right now, Xzibit and Rockwilder fall into this category; a few years ago it was Canibus, and in the early 90′s just after the birth of Cypress Hill, it was DJ Muggs. In 1992, finding a Soul Assassins remix on the back of say, a Beastie Boys 12″, was just as common as finding one on the b-side of a single from Da Lench Mob, ironically enough.
But, as time passes, and the industry decides that you're not "hot" anymore, those opportunities to do remixes and guest shots stop coming around, just ask The Beatnuts or Pete Rock. Nevertheless, while the Soul Assassins weren't being tapped for remixes after Cypress Hill's success with "Insane In The Brain" and their second album, Black Sunday, it didn't stop Muggs from making killer beats for everyone involved. The often fronted on House of Pain and Funkdoobiest built careers off Muggs' brilliant beats, both who coincidentally fell the fuck off after he stopped producing for them. After Cypress Hill began to lose popularity with their third release, Muggs managed to still keep heads ringing with the original Soul Assassins compilation, a joint effort between himself and silent collaborator, The Alchemist, which turned out some incredible collaborations with members of The Wu-Tang Clan , Goodie Mob , Dr. Dre and even bringing out the ol' tiger in MC Ehit.
Muggs' follow-up disc attempts to create the same magic found on the slept on debut release, and does so, but not without fault. First let it be said that two of the potentially greatest songs of the year are included on this album, and are worth the price of the album alone. Muggs sets up about-to-blow emcees Kool G Rap and Xzibit beautifully on both "Real Life" and "You Better Believe", respectively. These two tracks show what happens when incredible emcees rhyme on incredible beats, evoking the musical equivalent of fire.
Yet, this album is at times awkward, such is the case on the GZA/Genius featured "When The Fat Lady Sings", one of Muggs' new keyboard fueled tracks that seems a bit out of place next to a majority of sample driven grooves. Other times it's hard to fully absorb Muggs gorgeous production, as the listener is stuck trying to get used to the new voices of oddball members of Infamous Mobb , Screwball , and the Cali underground.
But when the pros get on, it's all gravy. Goodie Mob blend right in Muggs' production, serving up a tasty dish of blunted soul food on "This Some'n To". The ever-improving Dilated Peoples lend their talents to the obvious Alchemist banger "Suckers Are Hidin'", that builds itself up with an addictive cymbal pattern. The spaghetti-westernized sound creeps in on both B-Real's "Don't Trip", and Kurupt's "When The Pain Inflict", making both artists shine their brightest yet.
But just as Kurupt stands out on the aforementioned cut, he sounds completely out of place on the pointless "Armageddon" interlude. This in fact is the defining condition of the entire album. When it's hot, it's hot – but when it's not, it's not. Truth be told, you'll find beautiful beats on this album, and in fact some of the strongest tracks of the year on it, you just may have to sift through a few weirder selections to get there. But given that this is an album spotlighting production rather than rhymes, the quality is there, and the Soul Assassins brand name should have no problem reappearing on b-sides everywhere.
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The Pharisees were a Jewish sect from the second century B.C. to the first century A.D. They considered the entire Old Testament to be authoritative--unlike the Sadducees who only accepted the first five books. The Pharisees believed in life after death, the resurrection, the existence of angels and demons, and that the way to God was through keeping the law. "According to Josephus, the Pharisees were the group most influential with the people, were noted for their accurate and therefore authoritative interpretations of Jewish law, and had their own traditions and way of life to which they were faithful. They had a simple standard of living and cultivated harmonious relations with others.1
"And He also told this parable to some people who trusted in themselves that they were righteous, and viewed others with contempt: 10 "Two men went up into the temple to pray, one a Pharisee and the other a tax collector. 11 The Pharisee stood and was praying this to himself: 'God, I thank You that I am not like other people: swindlers, unjust, adulterers, or even like this tax collector. 12 'I fast twice a week; I pay tithes of all that I get.' 13 "But the tax collector, standing some distance away, was even unwilling to lift up his eyes to heaven, but was beating his breast, saying, 'God, be merciful to me, the sinner!' 14 "I tell you, this man went to his house justified rather than the other; for everyone who exalts himself will be humbled, but he who humbles himself will be exalted," (Luke 18:9–14).
- 1. "Achtemeier, Paul J., Th.D., Harper's Bible Dictionary, (San Francisco: Harper and Row, Publishers, Inc.) 1985.
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Phone (508) 807-0825
Age Suitability All Ages
Winter Trunk Show - Jewelry
Friday, Feb 1, 2013 9:00a to 5:00p
Fleur-tatious Floral Design Bridgewater, MA
Fleur-tatious Floral Design welcomes local jeweler, Shannan Nilz, to our shop to share her jewelry in a Winter Trunk Show event. Join us for light refreshments, flowers, and lots of gorgeous jewelry!
Shannan will be on hand to tell the story of how she came to be a jeweler and share the inspirations and motivations behind her work. All work displayed at the show is available for purchase.
Created by sn_studio
Location & Nearby Info
Fleur-tatious Floral Design
985 Pleasant St.
Bridgewater, MA 02324
985 Pleasant St.
Bridgewater, MA 02324
Show nearby:
1.7 mi 2 Barrett's Alehouse
1.7 mi 4 Chatta Box
1.7 mi 5 Baldie's Pizzeria
2.1 mi 7 Bruno's Pizzeria
2.2 mi 8 Crispi's Italian Cuisine
2.4 mi 9 Marylou's
2.5 mi 10 Riviera Cafe
Reviews & Comments
Hot Tickets More »
Sat 7/4 10:00a
Fri 8/28 7:30p
Tue 8/18 7:30p
Sat 3/14 7:30a
Fri 5/22 10:00a
Thu 3/26 6:00p


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Miss Smith
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Replied To: Live Webchat with Trey TONIGHT! (Blog)
On: Oct 11, 2011
Loving my calendar!!! So glad it was brought back =)
Replied To: We Want to Hear from You! (Forum topic)
On: Feb 16, 2011
Restock the calendars please & thank you =)
Replied To: We Want to Hear from You! (Forum topic)
On: Feb 02, 2011
I love him on Gucci's song Beat it up! He did the hook and it sounded awesome!! Oh and Sex Room with Ludacris ah just too sexy love it!!
Replied To: WHAT'S UR FAVORITE SONG FEATURING TREY SONGZ? (Forum topic)
On: Jan 21, 2011
Okay seriously please restock the calendar!! It's not like they won't get sold. Think about all of the fans that are a part of treysongz.com & they're going to tell their friends about it too. Please restock I really want one!!!!!
Replied To: **TREY SONGZ CALENDAR IS SOLD OUT** (Forum topic)
On: Jan 21, 2011


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Plumbers and HVAC specialists were busy Monday as they geared up for an anticipated onslaught of problems from the arctic chill moving through the Charlotte area Tuesday.
"During these cold snaps, we get inundated," said Jim Bridges, owner of Gastonia-based Plumbing Connection. "We're not used to these kinds of temperatures."
So while the coldest temperatures to hit the area in a decade have many people hunkering down, these businesses are staffing up.
Morris Jenkins, a Charlotte-based company that provides air conditioning services and furnace repair, is expecting up to 1,200 calls. That's three to four times the number they'd normally get on a Tuesday in the winter, said spokeswoman Casey Welch.
Service manager Jonathan Bancroft says Morris Jenkins boosted weekday call center personnel and asked 71 service technicians and 24 installers – nearly all of the weekday and weekend staff – to be ready to work Tuesday.
Customers' cold-weather grievances run the gamut, from clogged filters to burst pipes, frozen drain lines to malfunctioning furnaces. The bottom line, many service providers say, is that Charlotte residents, accustomed to mild winters and light jackets, aren't well-acquainted with the preventive tactics.
For example, plumbers recommend that when temperatures fall below freezing, you should close crawl space doors tightly, open cabinets underneath sinks to let heated air touch the pipes, and keep faucets dripping at night to help prevent the pipes from freezing. And they all say routine maintenance is important.
"They wait for it to break, and then our phones ring off the hook," says Scott Shelton, owner of Charlotte Comfort Systems.
On Tuesday, Shelton says all five of his technicians will be working, as he expects at least three to four dozen calls – significantly more than the six to 12 calls he gets on a normal winter day.
Most calls will be emergency-oriented, he said, but some will be for regular maintenance. A service call is $90, Shelton said, and the repair cost could run from less than $100 to $1,000.
Local plumber Brian Long, who currently works solo, said he's spent the last month looking for another plumber to hire. Cold snaps often make for downed power lines, so in addition to the maintenance calls "I spend a lot of time installing gas logs, so people have some kind of heat source," Long said.
McMillan Portillo: 704-358-6045 On Twitter: @cbmcmillan
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In the past, exceeding on the AIMS testing meant that Arizona high school students could qualify for free tuition at one of the three Arizona universities. Now that the scholarship has been slashed by about three-fourths the original amount, some East Valley high schools are supplying students with their own incentives to encourage high test scores.
Beginning with last year's sophomore class, Corona del Sol High School in Tempe introduced an Incentive Reward Program tied to the Arizona Instrument to Measure Standards. Sophomores that exceed on two of the four AIMS tests qualify for one of the four rewards options: preferred parking, fine arts pass, couple's ticket to prom or an off-campus lunch ID for the student's junior year. Students in Corona's special education program also qualify for the reward program if they exceed on one of the tests.
"Anything that the schools can do to motivate the students to do well, they're going to do because the student achievement is our number one objective," said Lina Littell, director of communications for the Tempe Union High School District.
Scores from the AIMS tests are reflected in each high school's report card published by the Arizona Department of Education. The report card is a way of displaying a school's success rate, Littell said.
"If you as a parent see a school that has lower test scores and another school that might have higher test scores, where would you tend to want to put your child?" Littell said.
Littell said the state has also stopped funding AIMS tutoring. Tempe Union High Schools are continuing to fund some AIMS tutoring programs using money from their maintenance and operations budget.
"They've implemented tutoring programs on their own to assist and motivate students to exceed on the AIMS test," Littell said.
Desert Ridge High School, a Gilbert Public School in Mesa, is offering an academic incentive for exceeding AIMS scores. Students who retest to exceed in the fall and achieve an exceeding score will be able to drop a low test score in one of their classes for that semester, said Brandie Harris, director of assessment and accountability for Gilbert Public Schools.
The biggest difficulty for Gilbert Public High Schools is encouraging students that met standards on their first attempt at the AIMS to retest to try to exceed standards, Harris said. In the past, students would retest so they could receive the AIMS scholarship.
"That was a big incentive for kids and it's unfortunate that that's not there anymore," Harris said.
Harris said schools across the Gilbert Public School District are also planning "exceeds celebrations" for students who exceed on the retesting when results come in at the end of October.
Other schools haven't found a need to implement new incentives.
Ken James, principal of Chandler's Basha High School, said teachers don't talk to students about passing the AIMS test: their sights are always set on exceeding. James said that they compare Basha to other high schools to motivate the students to always do their best.
"They want to kind of have the bragging rights," James said. "Fortunately we've done pretty well. The students don't want to be the group that lets the school down basically."
James said the only time an incentive may come into play is if an individual teacher chooses to look at the AIMS scores and use that information accordingly.
"If a student stays right on the borderline maybe between an A or a B, sitting there at 89 percent, if they get that exceeding they may give them the benefit of the doubt and go up to the 90," James said.
Terri Wattawa, principal at Williams Field High School, located in Gilbert and part of the Higley Unified School District, said they are looking at the possibility of including incentives but have yet to make a decision. Wattawa said that some other schools in the Higley Unified School District have given prom tickets and other incentives to students who exceed.
Wattawa, said it is now harder to encourage students to exceed, but that some students are still reaching for the AIMS scholarship, even if it has decreased in value.
"Ideally, students want to have excellent test scores and achievement itself is the incentive so we haven't nailed anything down yet," Wattawa said.
Jessica, a junior studying journalism at ASU's Walter Cronkite School of Journalism and Mass Communication, is an intern with the Tribune this semester. She can be reached at firstname.lastname@example.com or (480) 898-6548.


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Kevin Willard
2014-15 Season Preview: College Coaches on the Hot Seat
Oct 7, 2014, 10:00 AM EST
Every season, a few college coaches find themselves on the Hot Seat as the season begins. Can they win themselves off in 2014-15?
Seton Hall officially hires Isaiah Whitehead's HS coach
Sep 9, 2014, 1:56 PM EST
This was a move Kevin Willard had to make.
Seton Hall will face more non-conference challenges in 2014-15
Jun 30, 2014, 5:50 PM EST
With the addition of a deep recruiting class, Seton Hall will challenge itself with more difficult non-conference games in 2014-15.
Report: Seton Hall lands late 2014 commitment from forward Michael Nzei
May 19, 2014, 11:20 AM EST
Seton Hall pulled in a late commitment from 2014 forward Michael Nzei on Monday morning.
Seton Hall center Eugene Teague poised to return Saturday
Jan 16, 2014, 6:05 PM EST
As was the case last season, the Seton Hall Pirates have been unable to avoid the injury bug for much of the 2013-14 season. Patrik Auda, Fuquan Edwin and Aaron Geramipoor all missed time due to injury, and the same went for senior center Eugene Teague after he suffered a terrifying fall in the Pirates'…
Seton Hall facing several injuries heading into game against Creighton
Jan 4, 2014, 10:45 AM EST
The injury bug continues to strike Seton Hall and head coach Kevin Willard, as the Pirates have several players on the mend going into today's Big East home game against Creighton. According to J.P. Pelzman of NorthJersey.com, Seton Hall will make a game-time decision on senior center Gene Teague and senior wing Fuquan Edwin before…
Vin Parise's 30-second timeout: Five questions with Kevin Willard
Jan 3, 2014, 10:28 AM EST
Vin Parise of College Basketball Talk caught up with Seton Hall head coach Kevin Willard, who is 1-0 in league after the start of Big East play: CBT: Let's start off first with your 81-80 double OT win at Providence on New Year's Eve. Willard: Going in I was hoping we could try and steal…
Seton Hall rolls past Lafayette, Gene Teague suffers scary injury to head
Dec 27, 2013, 10:40 PM EST
The result of tonight's game between Seton Hall and Lafayette was never in doubt. The Pirates got out to a 47-15 lead at halftime, and the only question was whether they would double up Lafayette's score. They didn't, but the final score was 90-58 — a true throttling from the opening tip to final buzzer.…
Seton Hall PG Sterling Gibbs to return against Lafayette
Dec 27, 2013, 12:30 PM EST
Thirteen days ago when starting point guard Sterling Gibbs went down with a knee injury in Seton Hall's overtime loss to Saint Peter's, fans feared the worst. With Fuquan Edwin (ankle) and Patrik Auda (foot) already dealing with health issues, Kevin Willard's team could ill afford another injury to one of the key members of…
Seton Hall loses guard Sterling Gibbs to a knee injury
Dec 14, 2013, 5:33 PM EST
The news for Seton Hall continues to go from bad to worse as the Pirates not only lost a home game in overtime to struggling St. Peter's on Saturday, but they might have lost sophomore guard Sterling Gibbs to a knee injury. According to Jerry Carino of New Jersey Hoops Haven, Gibbs went down with the…
Win over LIU Brooklyn comes at a cost for Seton Hall as Fuquan Edwin goes down
Dec 5, 2013, 11:15 PM EST
Seton Hall established a season high for points in a game on Thursday night in their 92-81 win over LIU Brooklyn, with Brian Oliver knocking down eight three-pointers and scoring a game-high 26 points to lead the way offensively. In total four Pirates scored in double figures, but the win may have come at a…
Report: Tom Maayan to leave Seton Hall to rejoin to Israeli military
Nov 19, 2013, 6:05 PM EST
Tom Maayan was told on Monday, following Seton Hall's 82-66 win over Monmouth, that his sophomore season with the Pirates may have ended. According to a report from Zach Schonbrun of the New York Times, Maayan may have to leave the basketball program and return to Israel by Jan. 2 to fulfill his military obligation.…
Seton Hall coach Kevin Willard will compete in hot dog eating contest with Kobayashi
Oct 21, 2013, 10:35 PM EST
Kobayashi's six-year reign as Nathan's Annual Hot Dog Eating Contest took place on the corner of Surf and Stillwell Avenues in Coney Island. The former hot dog eating champ is taking his talents to South Orange on Oct. 25, competing against Seton Hall head coach Kevin Willard and women's head coach Tony Bozzella as part of…
Seton Hall unveils new jerseys for this season (PHOTO)
Sep 24, 2013, 4:54 PM EST
Times are good for the Seton Hall men's basketball program, and that's been a rarity for a long time. The Pirates are entering the brand-new Big East with their eyes on the heralded Class of 2014 coming in. Seton Hall uprooted Brooklyn native Isaiah Whitehead last week when he picked SHU over St. John's, giving…
Isaiah Whitehead, No. 14 in Class of 2014, commits to Seton Hall
Sep 19, 2013, 3:37 PM EST
After a wild recruitment that saw some fireworks down the stretch, the latest in a long line of Brooklyn-bred, Lincoln HS stars finally announced where he would be attending school on Thursday afternoon. "I'd like to announce that I'll be taking my talents to Seton Hall University," Isaiah Whitehead, the No. 14 recruit in Rivals…
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Office of the Registrar
Office of the Registrar
Change Majors, Add Minors, Concentrations
Students who want to change or add majors, minors and career concentrations need to fill out the appropriate paperwork at the Office of the Registrar, Student Services Center 150. For minors and career concentrations paperwork will then need to be taken to the academic department for their signature. What majors need permission?
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BU's Office of the Registrar is the central office for student scheduling and registration, as well as commencement, college transcripts, scheduling, undergraduate degree clearance, enrollment verifications, military credits, transfer credits, changing of a major, declaring a minor, and processing declaring a concentration.
Final Grading Information for Fall 2014
Final grades for the Fall term will be available for students in ISIS on or before December 19. For assistance on how to view your grades please click on the link below. Students are reminded that "I" and "X" grades from the Spring and Summer 2014 semester that have not been cleared will be turned to "F" grades. Please contact the instructor of your class to have a grade submitted via a grade change form. No grade reports are sent to students via hard copy. Official transcripts can be requested in your ISIS Student Center, from the other academic drop down menu choose – TRANSCRIPT: REQUEST OFFICIAL.
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Once final grades are posted, those students who fail to meet the good academic standing criteria are subject to probation or dismissal from the institution. The relevant academic policies and information may be found at the following links:
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Students are required to view their grades via the ISIS/PeopleSoft application. Failure to review grades via ISIS/PeopleSoft is not considered to be a reason for appeal of dismissal from the institution. Failure to have a current and accurate address on file in the Office of the Registrar is also not considered to be reason for an appeal of dismissal from the institution.
Students who are dismissed from the institution are sent a certified letter and an email of dismissal from the Office of the Registrar. These letters will be mailed to students the week of December 22, 2014. Students have the right to appeal. Appeals are due in the Office of the Registrar no later than January 2, 2015. Letters of appeals should be emailed as well as a hard copy sent to the Office of the Registrar.
Students who have an "I" or "X" grade are evaluated for academic standing and are still eligible for probation or dismissal based upon the remaining grades posted to their record.
New Transfer Course Equivalency Application
The course equivalency application is designed to allow students and advisors to look up a course at another institution and immediately see the Bloomsburg Equivalency. Prior to coming to the Office of the Registrar to complete a Prior Approval form, use this application to determine what the Bloomsburg Equivalency will be.
Always meet with your academic advisor for specific information concerning transfer courses and their application to your degree requirements.


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Written on: 24/08/2010
I wouldn't give them any stars except your system obliges me to do so!
I went to the local Post Office a year ago to buy 1000 euros. I was told that a travel money card would be safer and could be used anywhere, just like cash. I activated the card then went off travelling for a year. The card never worked and I gave up trying. When I returned to UK and asked for my money back they said I must give them £5.00 to 'redeem' it. This is fraud or at least a missold financial instrument.
What to do to get back the full amount?
As rated by real users
" Use different organisation " Read More
" Warning Do NOT Buy! Impossible to cash/use! " Read More
" Can't even get them back in my home country " Read More
" Confused " Read More
" Worked prefectly for our trip to Orlando in 2010 for both myself an... " Read More


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|RoM Quicklinks: News • Guides • Zones • Quests • Mobs • Items • POIs • Objects • Classes • Factions • Skills • Lore • Titles
|Help • SiteMap • Admin Pages • Templates
In this window is where all the upgrading will take place. Here's what you can do:
If you have 3 mana stones, you have 2 choices:
When the combination is right, a preview will be shown at the bottom of the Transmutor screen.
There are two ways to make runes using the Arcane Transmutor:
Bonus: After doing this, you can upgrade more by adding runes to the weapons, and even more using the upgrade jewels.
|ZAM would like to thank Official Runes of Magic Forums for some of the information in this article.
This Guide was originally a post at Evil Kittens, by likwidsage, during Open Beta. The site no longer exists.


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Stilettos aren't just for your heels anymore -- because super-sharp nails are starting to get seriously popular!
Rihanna, Lady Gaga and Katy Perry are just some of the fierce fashionistas rocking the stiletto nail these days -- so start filing your claws and get with the latest trend!
I would be afraid of accidentally poking my eye out with these!
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The AD1836A is a high performance, single-chip codec that provides three stereo DACs and two stereo ADCs using ADI's patented multibit Σ-Δ architecture. An SPI® port is included, allowing a microcontroller to adjust volume and many other parameters. The AD1836A operates from a 5 V supply, with provision for a separate output supply to interface with low voltage external circuitry. The AD1836A is available in a 52-lead MQFP (PQFP) package.
|Content Type
|File Type
|AD1836A: Multichannel 96 kHz Codec Data Sheet (Rev A, 01/2012) (pdf, 2288 kB)
|Data Sheets
Benchmarking Integrated Audio: Why CPU Usage Alone No Longer Predicts User Experience
(pdf, 1052 kB)
(www.analog.com/everywhere, 2007)
|Technical Articles
ASUS P5N32-E SLI Plus: NVIDIA's 650i goes Dual x16
(pdf, 3028 kB)
(AnandTech, 04/02/2007)
|Product Reviews
Realtek Audio Codecs Not Rendering True EAX
(pdf, 138 kB)
(DailyTech, 09/26/2006)
|Product Reviews
Music Synthesizer
(Design News, 7/17/2006)
|Product Reviews
The World is Still Analog
(Test & Measurement World, 6/1/2006)
|Product Reviews
Underneath Microsoft's Universal Audio Architecture
(pdf, 250 kB)
(DailyTech, 01/30/2007)
|Product Reviews
Audio Performance
(pdf, 811 kB)
(AnandTech, 10/20/2006)
|Product Reviews
|RAQs index
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|Glossary of EE Terms
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|AD1836 Sound CODEC Linux Driver
|Device Drivers
Symbols and Footprints— Analog Devices offers Symbols & Footprints which are compatible with a large set of today's CAD systems for broader and easier support.
The USA list pricing shown is for BUDGETARY USE ONLY, shown in United States dollars (FOB USA per unit for the stated volume), and is subject to change. International prices may differ due to local duties, taxes, fees and exchange rates. For volume-specific price or delivery quotes, please contact your local Analog Devices, Inc. sales office or authorized distributor. Pricing displayed for Evaluation Boards and Kits is based on 1-piece pricing.


text:
- Artist/Title: Nōh - s/t
- 6
- Format: 3inch CDR
- Label: Carbon Records
- Price: $6
- Catalog ID: CR158
duo of Larry J Patti (Foot and Mouth Disease) and Joe Tunis (Joe+N, Crush the Junta, Entente Cordiale, former-Pengo, etc), doing analog and electronic heavy/deep synth. [3" CDR housed in a LP cover, sprayed and stenciled. limited to 50 copies!]


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Me . . . JaneLittle, Brown Books for Young Readers 2012; US$ 9.99
In his characteristic heartwarming style, Patrick McDonnell tells the story of the young Jane Goodall and her special childhood toy chimpanzee named Jubilee. As the young Jane observes the natural world around her with wonder, she dreams of "a life living with and helping all animals," until one day she finds that her dream has come true. One of the... more...
The Very Fairy Princess Takes the StageLittle, Brown Books for Young Readers 2012; US$ 9.99
Everyone's favorite fairy princess is back and just in time for her ballet recital in this new picture book addition to the Julie Andrews Collection. At first, when Gerry is cast as the Court Jester and not the Crystal Princess, she is dismayed -- nothing is pink and no one can see her crown under her silly jester hat! But just as the recital looks... more...
The Very Fairy Princess: Here Comes the Flower Girl!Little, Brown Books for Young Readers 2012; US$ 9.99
Gerry is asked to be the flower girl in Aunt Sue's wedding, and she couldn't be more excited. Her imagination runs wild with thoughts of extravagant decorations, a billowy white gown, and hundreds of guests. When she finds out the bride prefers a small celebration, Gerry can't help but be disappointed... but she soon realizes that having the wedding... more...
The Very Fairy PrincessLittle, Brown Books for Young Readers 2012; US$ 6.66
While her friends and family may not believe in fairies, Geraldine knows, deep down, that she is a VERY fairy princess. From morning to night, Gerry does everything that fairy princesses do: she dresses in her royal attire, practices her flying skills, and she is always on the lookout for problems to solve. But it isn't all twirls and tiaras - as every... more...
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By AP/KWMU
Springfield, Ill. – Aides to Rod Blagojevich say the Illinois governor will use his first State of the State address to propose a comprehensive prescription drug plan for Illinois' seniors.
The plan would pool the purchasing power of nine state agencies that currently purchase drugs. Spokeswoman Cheryl Jackson says the nine agencies currently spend about $1.8 billion on prescription medication; but says combining the programs and purchasing in bulk would save $60 million a year.
Jackson said Blagojevich will also seek federal funding to expand the state's Circuit Breaker pharmaceutical subsidy program for low-income seniors.
St. Louis Public Radio
is a service of the University of Missouri-St. Louis.


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Sunday, December 21, 2014
Follow us:
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SYRACUSE, N.Y. -- Syracuse Police are looking for a man accused of shooting a dog at a house party. It happened at a party on the 200 block of Amhurst Avenue a little after 7:30 a.m. Sunday.
Police say an argument started over payment for the DJ. When the fight spilled out into the street, someone brought out a pit bull. Police say a man shot and killed the dog.
One man was also hurt during the fight. Police say Jamil Washington was taken to Upstate University Hospital with non-life threatening injuries.
Anyone with information on the shooting is asked to call police at (315) 442-5222. All calls will be kept confidential.
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Samsung Galaxy Tab 10.1 getting TouchWiz soon with Honeycomb update
Having a custom skin on top of the vanilla Android build has often proven to be more of a hassle than a real benefit. But while Samsung's TouchWiz UI won't appeal to Android purists, even they'd admit it does extend Android's functionality. The skin is now coming to Samsung's ultra slim Galaxy Tab 10.1 bringing advanced copy-paste storing images and links in the clipboard for easy sharing, a panel for quickly controlling settings like Wi-Fi and notifications, but also a new visual approach to multitasking with mini apps tray and live panel widget for magazine-like view of your most recent updates including weather and email.
The update also delivers Media Hub, a service allowing you to purchase and rent movies and TV shows, which you can subsequently share with other Media Hub devices. Samsung's Social Hub message aggregator, Reader Hub and Music Hub are also on board. The latest version of Swype comes preinstalled as well. With even more accessories like an SD card adapter, which the tablet has been notably missing, the Tab 10.1 should look even more appealing. Finally, if you lose your device, you'll be able to look for it, lock it or wipe out personal information. The update is coming soon, so it might arrive even sooner than the 4G LTE Galaxy Tab 10.1, expected to ship in the next couple of weeks.
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5 Comments
posted on 04 Jul 2011, 07:18 1
1. hawk62 (Posts: 320; Member since: 21 Nov 2009)
Wonder if it will fix the force close issue with this site? 99% of my browser's fc's have been on phone arena.
posted on 04 Jul 2011, 20:54 0
3. Galen20K (Posts: 517; Member since: 26 Dec 2008)
I've noticed if I use Opera Mobile on my 10.1 I don't have the force close issues with Phonearena.com.
posted on 06 Jul 2011, 03:35 0
4. awaes (unregistered)
i like this phone
posted on 15 Jul 2011, 11:07 0
5. Bantn (unregistered)
Oh, very good,http://aaaa.vn
Samsung Galaxy Tab 10.1 getting TouchWiz soon with Honeycomb update


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Hello fellow Texan, we have created a community just for Texas bloggers and would like for you to join. We have lots in store for the new year and the active members.


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11 ideas posted
35 comments 258 votes 105 users
In this community, you can submit ideas, vote on existing ideas, or add comments.
To submit an idea, please click the Submit New Idea button at the top of the navigation sidebar. You will then be asked to add a title and choose a campaign for the new idea. You will also have the option to add tags to the idea. To vote on an idea, simply click the up or down arrows to the right of the idea title/description. And to add a comment, click in the box below the idea.
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A Zotero app that allows researchers to import and organize digital images and upload to their citation libraries with metadata.
A serendipitous discovery tool for researchers that takes information from your personal collection (such as a Zotero citation library - http://www.zotero.org - or a CSV file) and delivers content (from online libraries or collections like DPLA - http://dp.la/ or Europeana - http://www.europeana.eu) similar to it, which can then be visualized and manipulated.
a web application for exploring and visualizing topics discovered within text content using the statistical method of topic modeling (possibly a wrapper for Mallet - http://mallet.cs.umass.edu/ - a common topic modeling tool). Aimed at technical novices unable to use Mallet's command-line tools.
A WordPress plugin for authors, editors and publishers to improve copyediting workflows for line editing, ideally with track changes functionality
A smartphone app that lets historians and teachers/students records and submit oral histories along with metadata.
a web- or desktop-based tool for linking images to an archival finding aid; and a plugin for Archives Space to populate collections with tagged images.
A web-based application for network analysis and visualizing complex relationships
A web application for users to arrange content of various types in ordered relationships, including timelines
A Wordpress plugin that lets teachers and other academics easily create and backup their own "Storify" on self-hosted Wordpress sites
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Thursday, December 18, 2014
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SCHENECTADY, N.Y. -- The 2012 March for Babies kicked off in Schenectady Sunday.
Close to 500 people gathered at Schenectady Community College for the three mile walk.
Organizers brought in lunch for walkers, and some family friendly activities for after the walk. GE collaborated with the March of Dimes to sponsor this year's walk.
The March for Babies is the March of Dimes' premier fundraising event. The goal of the organization is to improve the overall health of babies by preventing birth defects, premature birth and infant mortality.
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Jukka K. Korpela wrote: > It seems that [in HTML5 mode] the > validator reports any return statement inside an event attribute as an > error. Yet another example is that the following document is reported > to be in error: > > <!doctype html> > <title></title> >
foo
 The document now passes. I did some other tests too, and apparently the bug has now been fixed. -- Yucca, http://www.cs.tut.fi/~jkorpela/Received on Wednesday, 16 February 2011 06:42:07 GMT
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Clinic Floor- 586-200-6358 | Admissions - 586-200-6357 xt. 22
40688 Van Dyke Avenue Sterling Heights, MICHIGAN 48313 | FASFA CODE: E02118
By By Eric Czarnik C & G Staff Writer
Fri Nov 21 2014 at 5:54 PM
Talent show a hit with CSDD performers
Audiences were all ears when the world of Disney took the stage during a Nov. 7 talent show and fundraiser at Henry Ford II High School in Sterling Heights. During the show, an estimated 60 adult performers with disabilities acted, sang, danced and more. The performers came from Comprehensive Services for the Developmentally Disabled in Warren
By PM GIRLS
Mon Nov 10 2014 at 4:07 PM
Paul Mitchell Editorial Director and celeb stylist Lucie Doughty took simple braids and effortless waves to a new level in her recent editorial spread for American Salon magazine. And we wouldn't expect anything less! Lucie is known for creating beautiful styles that easily translate into everyday life for modern men and women. If you're on the hunt for fall hair inspiration, consider these noir-inspired looks.
By Paul Mitchell the School Michigan
Wed Oct 01 2014 at 5:02 PM
A Future Professional attends London Fashion Week
I was looking for schools for 3 months, was working at Macy's as a counter manager for cosmetics. And since I was doing hair at home, I figured I should just go to school for it. I could not find a school that had weekends off, so I quit my job, and than found Paul Mitchell and found that I could have Saturdays off and be able to keep my job as well.
By Connectus.Education
Wed Sep 24 2014 at 4:33 PM
3 Tips for Doing Shoots
3 Tips for Doing Shoots Creating collections and doing photo shoots is such a personal experience, that's what makes art so interesting, everyone has a different way of expressing it. What appeals to one person may not appeal to another, BUT there are a few tips Ruth Roche, Artistic Ambassador for Pureology Serious Colour Care, offers that can draw attention an image. Learn more about Roche and view her portfolio on ruthroche.com/portfolio/. "Everyone has their own style and talent when it comes to bringing a vision to life and shooting it, so you can't mess with that, but I know when I follow these tips, my work is elevated," says Roche.
By Paul Mitchell the School Michigan
Mon Sep 22 2014 at 6:44 PM
Wigs 4 Kids Gala
We had the pleasure of presenting a check to the Wigs4Kids foundation on September 18th on behalf of all of the Paul Mitchell Schools in the network in the amount of $25,000 and we also had a surprise to the organization by donating another $3,950 from Paul Mitchell the School Michigan.
By Launchpad Magazine
Wed Sep 17 2014 at 3:28 PM
Charity Begins at Home!
In the past 11 years, the international network of Paul Mitchell cosmetology schools has raised and donated over $13.3 million to a variety of charitable organizations, including $1 million to Children's Miracle Network Hospitals, $1 million to Leeza Gibbons Memory Foundation, $410,000 to the Gary Sinise Foundation, $270,000 to Habitat for Humanity, and $680,000 to Food 4 Africa, to name just a few.
By Sarah Kobeski
Fri Aug 29 2014 at 2:18 PM
Giving back has always been our style! Whether that means taking steps toward sustainability, helping families in need or supporting underserved kids, Paul Mitchell® believes in doing good for people and our planet, and we know our fans do too.
By Paul Mitchell the School Michigan
Tue Aug 05 2014 at 8:05 PM
Remembering 9/11
Every year since the tragic attacks on September 11, 2001, Paul Mitchell cosmetology schools across America have held some type of event in remembrance of the precious lives lost that day. Some schools have hosted fundraising events for local police, firefighters, their widows and orphans funds, and even for rescue dogs. Other schools have held special in-school tributes or memorials that day. At our school we have decided to give away free services for the month.
By By Maggie Mulhern from Modern Salon
Tue Jul 22 2014 at 6:22 PM
5 TIPS On HOW TO Get Attention On Instagram
MODERN found Cassandra McGlaughlin when trolling instagram. This owner of the Platinum Salon in Tampa, Florida, and Paul Mitchell National Color Educator, wisely (and nicely) comments on the work of others, and also tags and mentions @MODERNSALON in all of her posts. How could we ignore her? Once we reached out to her, she responded immediately and allows herself to be highlighted. With her amazing and organic success, MODERN felt she would be the perfect person to offer tips.
By Paul Mitchell the School Michigan
Thu Jun 26 2014 at 2:55 PM
Fernando Adame is making moves with Kelly Cardenas
Fernanando graduated in 2014 and is pursuing his dreams! Check out his journey and story!!
By Stacey Soble from Modern Salon
Thu Jun 26 2014 at 1:52 PM
Millennium Experience 2014: Game On!
As salon owners, stylists and guest coordinators took their seats at the 2014 Millennium Experience in Ft. Lauderdale, Florida, an electronic voice encouraged them to take out their phones, log onto playTME.com, take their place on one of four teams and tap their phones as quickly as possible earning points for the team. The engaging activity immediately enrolled this year's attendees into Millennium Systems International Founder John Harms' "Game On" theme for the year.
By By Lauren Salapatek from Modern Salon
Fri Jun 20 2014 at 7:54 PM
7 Elegant Special Occasion Looks For a Wedding or Formal Party
Inspired by stars on the Red Carpet like Taylor Swift, Jessica Alba, Beyonce, Kim Kardashian and Tyra Banks, Lizzie Liros created a hair collection of "Red Carpet" looks that are both beautifully unstructured and textured.
By Paul Mitchell the School Michigan
Fri Jun 13 2014 at 4:36 PM
Introducing the Ultimate Deep Cleansing Shampoo: Heavy Hitter™
Introducing the Ultimate Deep Cleansing Shampoo: Heavy Hitter™
By Gail Fink
Fri Jun 13 2014 at 4:30 PM
PBA Announces 2014 Beacon Winners
The Professional Beauty Association (PBA) announced the winners and honorable mentions of its 2014 Beacon competition, and nearly half are from Paul Mitchell Schools. Beacon provides the nation's most promising cosmetology students with education and opportunities to network with the industry's highest profile salon owners and stylists during PBA Beauty Week, July 12-14, 2014 in Las Vegas. Beacon students attend specialized classes with the biggest names in the industry, get up close and personal with NAHA finalists, and get a firm understanding of the business of beauty.
By Paul Mitchell the School Michigan
Fri May 23 2014 at 7:10 PM
Yesterday marked the first ever #tinablcakday our Owner Tina Black was recently diagnosed with a precancerous condition in her uterus called complex hyperplasia only detected by a biopsy and not by a routine papsmear. Uteran and ovary cancer is the most aggressive of all cancers because they are difficult to detect. But www.brightpink.org is raising awareness for such cancers. Tina said that she is blessed to have found it so early. Bright Pink is more than just a color. It is a movement, a community, a way of life. It is the belief that being proactive is better than being reactive, that prevention is better than treatment. Educate yourself, take action, and join us in Being Bright Pink.
© 2013 Paul Mitchell Advanced Education
Website Developed by Robinsage
Website Developed by Robinsage


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Dallas Review: Making Daddy Proudby Christine Orlando at . Comments
The original Dallas started off with one major theme. It was about two brothers who desperately wanted to make daddy proud. Fast forward 30 years and you'll find that not much has changed.
Let's review the latest episode, shall we?
J.R. Comes Home. "The Price You Pay" opened with J.R. holding a blade to his son's throat. No need to call the cops. It was just J.R.'s way of showing the boy he cared.
You could tell that J.R. was more than a little proud of his child's ability to go behind his back, even if he didn't quite pull it off. And despite being all grown up, John Ross was desperate to win his father's approval.
That was quite some piece of theater they pulled off in front of Bobby and Annie as they squabbled over Miss Ellie's journal. It was good, just not good enough.
Annie Get Your Gun. The more I see of Annie, the more I like her. When this woman sees trouble she picks up her gun and confronts it head on but as J.R. was quick to point out in this Dallas quote...
Bullets don't seem to have much of an effect on me darlin'. | permalink
She didn't hesitate about having J.R. move back into Southfork because he's family, yet she saw right through the old devil when he used his son to manipulate Bobby.
Now if she could only use that x-ray vision to see through Tommy and Rebecca the Ewings would be much better off.
Cliff Barnes Returns. I remember that there were moments when Cliff had a sweet side, especially when it came to his sister, but more often than not he was just a conniving fool. J.R. crushed him under his boot more often than not, yet the man kept getting up for more.
When J.R. was just as ornery to Cliff as he'd ever been, I had to smile. It's nice to see that some things haven't changed.
But has Cliff now been relegated to the role of Christopher's crazy old uncle. I was proud of Christopher when he turned down that money. As Cliff told him he'd never be a real Ewing and warned him not to let the Ewings destroy him the way they had Pam, it was clear that nothing has changed at all. The Barnes/Ewing feud lives on.
Everyone Returns to Southfork. One of the strangely dysfunctional and incredibly entertaining things about Dallas has always been how everyone migrates back to Southfork, even when they despise one another.
J.R. being back will surely give us many wonderful moments between him and Bobby but my favorite was when he showed Annie the photo of Bobby and Miss Ellie and told her...
Spent a lot of my life hating how much she loved him. | permalink
It's so true. So much of their issues come from the petty jealousies of children who never really grew up. Now Southfork is just the latest toy they're arguing over.
There were so many other moments in this episode that it's hard to list them all but here are a few…
- I was a little disappointed that Rebecca sent Elena that e-mail. It makes the most sense but I found myself hoping for an additional twist.
- It was almost comical that Bobby was more worried about hair loss than heart failure when it came to the side effects of his treatment.
- The Elena/Christopher/Rebecca love triangle gets more complicated every week and I love it even though I'm not even sure who I'm rooting for just yet.
- Can someone please trim J.R.'s eyebrows? They're so distracting I'm afraid they're going to crawl away on their own.
I'm already lamenting that there are only seven episodes left in this season because I'm having so much fun getting to know the Ewings all over again. How about you?
C. Orlando is a TV Fanatic Staff Writer. Follow her on Twitter.Tags: Dallas, Reviews
Loved the shaving scene. J.R. (as he shaves John Ross' throat with a very sharp razor): I loved my daddy, and I respected my daddy, but most important, I feared my daddy. … Were you gonna cut your daddy out of $2 billion dollars worth of oil? The look on John Ross' face was priceless. OMG! He knows! look on his face.
I laughed so hard when JR said he recognized the smell of "brimstone and crazy", I had to pause the episode. Also, the reminder that bullets don't seem to have much of an effect on JR? Priceless.
Finally, a return of the true, hard working - actors and not all that "reality" crap!
I love Dallas-then and now- however, there was a slight mention of
Pam just disappearing = does that leave the door open for her to
return ...I sure hope so.
Great writing... Keep it coming.
Long live J.R. and his "dastardly deeds"! Bless the old scoundrel's heart, he is never boring. Now if the other characters could be one quarter as interesting as him, Dallas would be quite a show ...
The show is getting interesting! there's no triangle for me, I'm definitely rooting for rebecca and christopher!
Agree with Rank. When JR's eyes opened and he said, "the fried chicken here isn't bad. Get me some of that red jello, too," I was much relieved.
Oh, I think Hagman should keep those brows. They make him look more devilish. It's almost like they're an additional character because they certainly get more attention than Sue Ellen. Everyone, including J.R., seems to forget that for all of J.R.'s dastardly deeds, Bobby ALWAYS found out and frequently bested his brother in business, usually because J.R.'s way of doing things got Ewing Oil in trouble with the government and sent them backwards to square one. I have two favorite scenea in this episode - the opening one w/JR & John Ross & the final one. Hagman & Josh are knocking it out of the park as father & spawn. Wow! Even when the dialogue is revealing there is so much going in on their expressions. Age is NOT slowing Hagman down one bit. When Bobby & Ann wryly comment about why J.R. even thinks he can fool them, we are reminded again that Bobby isn't just a good person; he's a survivor, and a very smart one. This is an EXCELLENT continuation of DALLAS. BRAVO! Keep it comin'!
Love the new episodes. I wonder if Valine and Gary will visit.
I think Rebecca will come clean in the next couple episodes to Christopher and that he'll stay with her because he feels guilty for kissing Elena.
Great episode. This show is living up to expectations. I'm curious to see where this show will dare to tread regarding JR teaming up with some serious unsavory types from South America. Nice to see Carlos Bernard, Tony from 24, back on tv. These guys seem like some serious kill you as quick as look at you types and will be interesting to see the JR we know deal with these "allies". A good thing is I'm actually digging the new generation which, is important for the show to have legs. I really like John Ross, Christopher and Elayna, not sold on Rebecca yet but will see how that plays out. Loving the new Dallas!!


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Boulder News
Local news for Boulder, CO continually updated from thousands of sources on the web.
Boulder cop's arrest this fall is 8th since 2011
11 hrs ago | LongmontFYI | Comment?
FERC: Boulder taking of Xcel transmission loop needs our approval
17 hrs ago | Daily Camera | Comment?
The guitar ninja comes but once a year
18 hrs ago | Boulder Weekly | Comment?
Smash and grab burglars strike two Boulder trailheads on Wednesday
18 hrs ago | Denver Post | Comment?
Q&A: Drones might help explain how tornadoes form
18 hrs ago | Norwalk Citizen News | Comment?
CU-Boulder police hire new deputy chief of support services
19 hrs ago | Daily Camera | Comment?
An independent fit for Boulder
19 hrs ago | Boulder Weekly | Comment?
21 things to do today, Dec. 18, in Boulder County
22 hrs ago | Daily Camera | Comment?
Boulder Google campus at Pearl, 30th moves forward
Yesterday | The Boulder County Business Report | Comment?
CU hopes to keep tuition increases in check again this year
Boulder beekeeper wants allowance for cottage industries
Yesterday | LongmontFYI | Comment?
Broadway to be narrowed while Boulder removes diseased oaks
Boulder County letter carriers deliver holiday mail during busiest time of year
Sen. Mark Udall nominates six Boulder-area students to military academies
Libyan refugee Iman al-Obeidi sentenced to work release for violating probation
Wednesday | Daily Camera | Comment?
Man tasered by CU-Boulder police after brandishing pen sentenced to probation
Wednesday | Daily Camera | Comment?
Updated: Fri Dec 19, 2014 04:06 am
Copyright © 2014 Topix LLC


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Staff are non-paid volunteers who work throughout the year and at con to make Anime Expo and Anime Conji what they are.
- Must be 18 years of age
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- Becoming a part of the close knit community of fans and friends
- Free staff specific swag (i.e. staff only t-shirt)
- Resume and experience building
- Basic food/housing provisions during the convention
- Behind the scenes look at how conventions and the industry are run
There are many different departments within SPJA-- over 10 for the Business Operations and over 30 specifically for Anime Expo. With over 1,500 volunteer staff, finding your home is important!
Divisions include: AV Tech, Interactive Events, Programming, Guest Relations.Department descriptions coming soon!
Divisions include: Facilities, Attendee Services.Department descriptions coming soon!
Divisions include: Marketing, Technology, Staff Resources, Accounting.Department descriptions coming soon!


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Home → Sports→ BGSU
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Most Recent Articles In Lifestyle
Latest Lifestyle Articles
Finding the Long March Canteen might feel like a trek or even a trick — the dim sum spot is somewhat hidden behind its playful exterior, including a faux-barricaded door, wild graffiti, and, currently, scaffolding. But inside, the food doesn't mess around. This sister restaurant to dumpling spot Yumcha Heroes offers some of the same dishes, but adds the mix-and-match fun of choosing cold dishes a la carte — and from a cart. Friendly wait-staff wheel an array of small plates, including succulent seared tuna with red beets and edamame, honey-glazed spare ribs, silken tofu with thousand-year-old eggs and preserved vegetables and jellyfish carpaccio. Cold dishes run 5 to 9.50 euros, or about $6 to $12.
Warm dishes supplement the cart's instant gratifications — crispy tofu with salt, chili, garlic and Thai basil, grilled baby squid, pork belly with baby asparagus and Peking duck. Hot dishes range from 6 to 15 euros, or about $7.50 to $19. Dumplings are available baked, steamed, or in soup, in a wide variety of fillings — meat, fish, and vegetable (4.50 to 7 euros, or about $6 to $9). Finish the meal with a chocolate version dressed with cinnamon and vanilla sauce (5.50 euros, or about $7).
The interior, designed by Ett la Benn — the team behind many of Berlin's best-dressed restaurants — plays with Sino-kitsch, but the open ceilings, family-style long tables, industrial lamps and chopstick dispensers keep everything on track.
Long March Canteen
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The Year Of Luigi
Limited Edition 2DS console planned for this, The Year of Luigi – report
Nintendo has made it very clear that this is The Year of Luigi. And now, following the lanky plumber getting his own 3DS XL console, it looks like he'll be lending his name to a Limited Edition 2DS console too. That's if leaked images are anything to go by, anyway.4


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Map of Fort Mims
A copy of a map of Fort Mims. This map was found among the papers of General Claiborne. Block house. Pickets cut away by the Indians. Guard's Station. Guard House. Western Gate. This Gate was shut, but a hole was cut by the Indians. Captain Bailey's Station. Steadham's House. Mrs. Dyer's House Kitchen. Mims' House.


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I spent some time today putting together a pre-alpha WebID specification. RDFa is an ideal fit for expressing information in the WebID document, so I put it in there as a normative requirement. This may change as I haven't talked with Henry Story or Toby on how they intended to express RDF in Web documents. My assumption was RDFa, but they may have had other things in mind. Here's the link to the e-mail announcement on payswarm-dev: http://payswarm.com/pipermail/payswarm-dev/2010-July/000035.html -- manu -- Manu Sporny (skype: msporny, twitter: manusporny) President/CEO - Digital Bazaar, Inc. blog: Myth Busting Web Stacks - PHP is Faster Than You Think http://blog.digitalbazaar.com/2010/06/12/myth-busting-php/2/Received on Sunday, 11 July 2010 21:29:21 GMT
This archive was generated by hypermail 2.2.0+W3C-0.50 : Friday, 27 April 2012 04:55:07 GMT


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Imagine if the company of Sleep No More the site-specific, immersive Macbeth takeoff still playing in NYC got to speak and sing. That's a close approximation of Red-Eye to Havre de Grace, New York Theatre Workshop's enthralling song-and-modern dance-laden depiction of the final, agonizing days of horror scribe Edgar Allan Poe (now playing through June 1). Though it's staged in a regular theater, Lucidity Suitcase Intercontinental and Wilhelm Bros. & Co.'s production is one of the rare experiences in which you feel separated from your body, as the fluid, dreamlike tableaux of Red-Eye take residence in your mind and firmly stay put.
Set mostly in Philadelphia (where it was previously mounted), Red-Eye begins with a cheeky prologue by Ranger Steve (cocreator/master tenor Jeremy Wilhelm, whose brother David provides musical backup). The ranger provides full-service background on the events leading up to the demise of Poe, played with consummate physical grace by the rubber-bodied Ean Sheehy, complete with a Chaplinesque mustache to complement his wiry frame. (Sheehy also works for People, a sister magazine of Entertainment Weekly.) We learn of Poe's past: He lost his teenage wife, Virginia, to TB; he's utterly devoted to his mother-in-law, 'Muddy' (who also happened to be his aunt); and he embarks on a harrowing train ride before ending up in a Baltimore hospital, gasping and delirious, and then succumbs to a (still) mysterious death at age 38.
Abjuring the standard approach for bioplays, director Thaddeus Phillips creates a stagescape not unlike one of Mr. Poe's celebrated stories. Virginia Poe (Alessandra L. Larson) becomes a wordless gypsy who literally floats (as in one jaw-dropping bit with an elevated bed) and slithers through the narrative in ghostly fashion, as our hapless Poe slowly crumbles before our eyes. Doors double as tables and vice versa, crawlspaces are created out of table legs, and a dancer finds new, elongated legs (I won't spoil the secret behind that marvelous visual nugget).
Phillips' expertly designed production also achieves a humane balance. Just when the material starts to lean toward the cerebral, the play's generously allocated sense of humor kicks in. For a dance-heavy piece about a dying author, Red-Eye is as fleet as a Wes Anderson comedy and conveys many of that celebrated filmmaker's same tropes. For instance, it is not above using a pop song to make a point. ''Neil Diamond pretty much says it all for me,'' says the sly Ranger Steve. (He's commenting on Diamond's ''Done Too Soon,'' which name-checks ''E.A. Poe.'')
At its best, this surreal and haunting play forces us to question the human experience in the modern age. ''Has all this speed made us more happy or more wise than we were 6,000 years ago?'' Poe asks. We're still figuring out the answer to that one, but the soulful, bravura Red-Eye to Havre de Grace will make you both happier and wiser. A
(Tickets: www.nytw.org)


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Very easy to use. You can charge your IPOD several times with only one charge. Very good product at a great price Muy facil de usar. Podes cargar tu Ipod varias veces con una sola carga. Muy buen producto a un precio excelente none ninguna I´ve been using it for 3 monts and it works great. I recomend ... Read more
Very beautifu, come in nice box with apple cable. Reached to my home in no time! I have an iPad and it's not powerful enough to charge it. I have a ballistic case, and it didn't feet to the case so I had to take of the case and than use it. Very sad it don't work with iPad. Very nice look like made from ... Read more
-The battery itself charges fast -Comes with the same cord that came with your ipod/iphone -Approximately 1.5 charges -With new IOS 5 you can wirelessly sych your device when its charging. - Not enough power to charge iPad It has a button and I'm not sure what it is used for. Overall, great product worth ... Read more
This is a very useful item, saved me more then a few times in emergency, it has a button that says the amount of baterry left inside, you can charge it with your regular apple charger. buy it if your not looking for one which will work as a panel also, it weight nothing and easy to carry it building ... Read more
- The price isn't to bad. - The quality is great, it seems like it will hold up against everyday wear and tear. - It has LED lights to indicate the battery level. - Really easy to use, it is just plug and go! - Great if you dont have a place to plug in your phone. (Camping, concerts, work, etc.) - Others ... Read more
- External battery with good quality build - Comes with LED indicators to show remaining battery life - Easily charged with standard iPod/iPhone USB cables - Can be charged with traditional walled power as well as computer USB power - Small and compact size is a bonus - Very light - Fits in pocket! -... Read more
- Package contains External Battery + iTunes cable (white, normal length) - Built quality looks okai - LED indicators - Easy for when you are travelling - Very light - Price is nice - Button for indication how full it is - No drivers have to be installed, works direct - No manual - Very thick in comparison ... Read more
Gets quickly recharged. Lightweight gadget for the 3GS. Recharges the iPhone battery 1.5 times and does it quite fast. Price is great! Bought two, one for a friend and another one for me. Unfortunately, my own stopped working after a week use time, and can't recharge it anymore. Good idea to buy more ... Read more
The 1800mAh USB Recharged Emergency Power Pack External Battery for iPod/iPhone/iPhone 3G -it can charge your ipod/iphone 1.5-2 times -easy to charge, just plug in the ipod charger -good build quality -led indicators -very usefull -very sturdy only that the plug doesnt give a satisfying click. - sometimes ... Read more
-It refills your iphone/ipod touch perfectly(i have an ipod 4g). -You can see when you need to refill your external battery. -Build quality is better than i expect. -Price is really low. -You can can refill you ipod 1.5 times with it. -It doesn't weight that much. -It is pretty big. -the cable which ... Read more


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Tag Archives: cover crops
20 Million Acres by 2020
When it comes to resiliency, cover crops are a no brainer! Although the temperatures are still cold outside, every farmer I know is busily planning their cropping season. Whether it's a vegetable grower firing up their greenhouse and anxiously awaiting … Continue reading


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Susan M. Pike, MD
Ratings based on 4 reviews
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Reviews (4)
5 out of 5 stars Tummy Tuck
Mom of Three in Her 40s Waited Long Enough for a TT - Round Rock, TX
First and foremost, I prefer to see a lady doctor because I feel more comfortable doing so. Secondly, Dr. Susan Pike has this very gentle and calm way about her that makes me feel safe and relaxed during my consultation. I felt safe to ask questions that I would not normally ask just because they sounded so unintelligent to me at that time (LOL!!). I felt safe to raise my concerns to her about what I really don't like about my body. She took the time to listen and examine me and gave me her opinion of what needs and need not be done for my case. In our discussion she came across as very confident and enthusiastic, that she knows what she can do to bring me to my goal and I have nothing to be worried or concerned about. Overall, I'm very pleased with how things are progressing so far.
2 out of 5 stars Brow Lift
exspected a better result - Round Rock, TX
First did not listen when I told her I got sick after surgery. DR PIKE ststed she hide the scar in a wrinkle in my forehead. It is not even close to hid.I will probly have the scar re-done.The Doctor did not hounor my last post op appt.Her receptinest said I was out of the 90 day post op. time limit which i had pre-paid. they made the appt. not me.Aso had drove 160 mile round trip for this apptment. I did not see the the DR.
5 out of 5 stars Breast Augmentation
My New Girls - Round Rock, TX
5 out of 5 stars Tummy Tuck


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35th Street & Broadway, Manhattan Island, Manhattan (New York Co.), New York City, New York, USA
Ref.: The Minerals of New York City & Its Environs, New York Mineralogical Club Bull., Vol. 3, No. 1, Manchester, J.G. (1931): 23.
35th Street & Broadway, Manhattan Island, Manhattan, New York City, New York, USA
Photo: 2008 Peter Cristofono
35th Street & Broadway, Manhattan Island, Manhattan, New York City, New York, USA
Photo: 2008 Peter Cristofono
Latitude: 40°45'0"N
Longitude: 73°59'17"W
Longitude: 73°59'17"W
Mineral List
| Almandine
1 entry listed. 1 valid mineral.
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Locality Updated: Veľká Poľana, Snina Co., Prešov Region, SlovakiaFrom Matúš Škutka, 22nd Dec 2014 12:56:29