Updated references in examples/NBodyAtmEsc.
@@ -16,16 +16,18 @@ envelope model to the N-Body module SpiNBody.
=================== ============
The orbital parameters are taken from `Konacki & Wolszczan (2003)
-<https://ui.adsabs.harvard.edu/abs/2003ApJ...591L.147K/abstract>`_. The properties
-of the pulsar from XXX. The luminosity of the pulsar is assumed to be 0.001
-L_sun, with all flux emitted in the XUV. These assumptions are consistent with
-YYY. The initial envelope mass of planet A is 1 Earth mass, while the core mass
-is 0.02 Earth masses `Konacki & Wolszczan (2003)
-<https://ui.adsabs.harvard.edu/abs/2003ApJ...591L.147K/abstract>`_. While such an
+<https://ui.adsabs.harvard.edu/abs/2003ApJ...591L.147K/abstract>`_. The
+XUV luminosity of the pulsar is assumed to be 0.001
+L_sun, which is about 3 times larger than the X-ray luminosity found by
+`Pavlov etal. (2007) <https://ui.adsabs.harvard.edu/abs/2007ApJ...664.1072P/abstract>`_.
+The initial envelope mass of planet A is 1 Earth mass, with a core mass
+of 0.02 Earth masses, which is the currently observed value `Konacki & Wolszczan
+ (2003) <https://ui.adsabs.harvard.edu/abs/2003ApJ...591L.147K/abstract>`_. While such an
initial composition seems unlikely, the large mass loss allows for the coupling
to be apparent in a simulation that requires ~1 hour to complete. Mass loss for
the B and C companions can occur of billion year timescales, see the
-`AtmEsc <AtmEsc>`_ directory.
+`AtmEsc <AtmEsc>`_ directory. The mass of the pulsar is 1.4 solar masses
+`Gozdziewski et al. (2005) <https://ui.adsabs.harvard.edu/abs/2005ApJ...619.1084G/abstract>`_.
To run this example
@@ -45,4 +47,5 @@ Expected output
**Top left**: Envelope mass of planet A. **Top right**: Radius of planet A.
**Bottom left**: Eccentricity evolution of all planets. **Bottom right**:
Inclination evolution of all planets. Note the second and third eccentricity
-cycles are lower than the first, which is due to A's mass loss.
+cycles are lower than the first, which is due to A's mass loss. Compare to Fig.
+1 in `Gozdziewski et al. (2005) <https://ui.adsabs.harvard.edu/abs/2005ApJ...619.1084G/abstract>`_.
