To the interested:
These files are a representative sample of raw M dwarf, brown dwarf, and giant planet models from Burrows et al. 1993 (Ap.J. 406, 158) and Burrows et al. 1997 (Ap.J. 491, 856). Masses of 0.01, 0.02, 0.03, 0.04, 0.05, 0.055, 0.06, 0.065, 0.07, 0.075-0.08, 0.085, 0.09, 0.095, and 0.1 solar masses, 1-9 Jupiter masses (.001-.009), and of 20 and 25 Jupiter masses are included (along with a few extras to taste).
The format is:
I, Time(Gyrs), Teff, Lumin, Rad(Gcm), Tc, Rhoc, S, Ratio, Yd, Ylithium,
where I is the step number, time is the age in gigayears, Teff, Lumin(solar), and Rad are clear, Tc and Rhoc are central values, S is the entropy of the convective core per baryon per Boltzmann constant, Ratio is the fraction of the radiation losses compenstated by nuclear burning, Yd is the deuterium fraction, and Ylithium is the lithium fraction. A few relaxation steps are allowed, so "Age=0" starts a bit down the file. Please refer to the papers above when using or quoting these data and please let me know if you do.