"Full evolution of low-mass white dwarfs with helium and oxygen cores"
Panei, J. A., Althaus, L. G., Chen, X., and Han, Z;
2007, MNRAS, 382, 779
CO-WD sequences with masses 0.3515, 0.3844, 0.3986, 0.4160 and 0.4481
M_sun. Ages are counted from the end of mass transfer.
M/Mo: stellar mass (in solar units)
log(L/Lo): logarithm_10 of luminosity (in solar units)
log(T_eff): logarithm_10 of effective temperature
log(t[10^6yr]): Log10( age (in 10**6 yr) )
R/Ro: radius of WD in solar radius
log(R[cm]): radius of WD in cm
log(g[cm/s^2]): logarithm_10( gravity (in cm/s^2) )