Cooling tracks for white dwarfs

with helium core

Cooling curves and initial models for low-mass white dwarfs (<0.25 Msun) with helium core
M. J. Sarna, Ene Ergma and Jelena Antipova
2000, MNRAS, 316, 84, Abstract, Table1a, Table1b, Table4a, Table4b

Z=0.003; Mi=1.0 Msun	Z=0.01; Mi=1.0 Msun	Z=0.02; Mi=1.0 Msun	Z=0.03; Mi=1.0 Msun
Z=0.003; Mi=1.5 Msun	Z=0.01; Mi=1.5 Msun	Z=0.02; Mi=1.5 Msun	Z=0.03; Mi=1.5 Msun

sarna@camk.ed.pl

Milky Way : Courtesy of HST : 1997 Releases