YaPSI

Isochrones are produced using the color tables of Lejeune, Cuisinier & Huber (1997), (1998); and the color tables and interpolation software of Worthey & Lee (2011)

Two stellar mass ranges considered: 0.15 < M/M_☉ < 0.90 and 0.60 < M/M_☉ < 5.00. Tracks constructed at mass dependent intervals.

Table of masses

1. model number
2. number of shells
3. age
4. X
5. Y
6. Z
7. log L/Lsun
8. log R/Rsun
9. log g
10. log Teff
11. mass coordinate at the top of the convective core (if present)
12. mass coordinate at the base of the outer convective envelope (if present; note: it is not the mass of the CZ!)
13. fractional radius at the bottom of the outer convective envelope (if present)
14. convective turnover time scale (days)
15. log temperature at the bottom of the outer convective envelope
16. surface X
17. surface Z
18. log central pressure (erg/cm2)
19. log central temperature (deg. K)
20. log central density (gm/cm3)
21. beta = Prad/P (radiation pressure parameter)
22. eta = (chemical potential)/kT (degeneracy parameter)
23. mass coordinate of the center of H burning shell (if present)
24. mass of the H burning shell (if present)
25. mass of the helium core
26. mass coordinate where the temperature maximum occurs
27. fraction of energy produced through gravitational contraction out of total energy produced (percent)
28. moment of inertia of the whole star (g cm^2)
29. moment of inertia of the outer convective envelope (if present)
30. moment of inertia of the convective core (if present)
31. luminosity generated by the ppI chain (erg/s)
32. luminosity generated by the ppII chain (erg/s)
33. luminosity generated by the ppIII chain (erg/s)
34. luminosity generated by the CNO cycle (erg/s)
35. luminosity generated by the 3-alpha reaction (erg/s)