Nicolaus Copernicus Astronomical Center: Marek J. Sarna:
Cooling
Cooling tracks for white dwarfs
with helium core
The binary stars at the beginning of mass transfer consist from 1.4 Msun
neutron star and 1 Msun red giant with small helium core (Mcore < 0.05
Msun).
In tables bellow we show cooling tracks for different white dwarfs masses.
The metalicity is Z=0.010 where Zcno= 0.0050.
Pi=1.30d;
Pf=0.366d; Mf=0.163Msun
