Stars), XINS (X-ray Isolated Neutron Stars), TEINS (Thermally Emitting Neutron Star), INS (Isolated Neutron Stars). Defined as thermally emitting neutron stars of high magnetic fields, although lower than that of magnetars. Identified in thermal X-rays, and thought to be radio-quiet. A group of seven individual, physically similar and relatively nearby neutron stars nicknamed The Magnificent Seven, consisting of: RX J185635-3754 RX J0720.4-3125 RBS1556 RBS1223 RX J0806.4-4132 RX J0420.0-5022 MS 0317.7-6647 1RXS J214303.7+065419/RBS 1774 Compact Central Objects in Supernova remnants Compact Central Objects in Supernova remnants (CCOs in SNRs) are identified as being radio-quiet compact X-ray sources surrounded by supernova remnants. They have thermal emission spectra, and lower magnetic fields than XDINSs and magnetars. RX J0822-4300 (1E 0820–4247) in the Puppis A supernova remnant (SNR G260.4-3.4). 1E 1207.4-5209 in the PKS 1209-51/52 supernova remnant (SNR G296.5+10). RXJ0007.0+7302 (in SNR G119.5+10.2, CTA1) RXJ0201.8+6435 (in SNR G130.7+3.1, 3C58) 1E 161348–5055 (in SNR G332.4-0.4, RCW103) RXJ2020.2+4026 (in SNR G078.2+2.1, γ–Cyg) Other neutron stars IGR J11014-6103: a runaway pulsar ejected from a supernova remnant. See also Neutron star merger Rotating radio transient IRAS 00500+6713 (in 10,000 y) Notes References Star types