15 files (.dat) with the name representing the initial mass (in solar mass, e.g. 0.8 is a 0.8 Msun)
In each of these files, there are 22 models with different initial helium from 0.248 (in mass fraction) to 0.8 -> [0.248,0.26,0.27,0.3,0.33,0.37,0.4,0.425,0.45,0.475,0.5,0.525,0.55,0.575,0.6,0.625,0.65,0.675,0.7,0.73,0.77,0.8]
Before each set of data, there is a header displaying the number of lines for each model (up to 500), the initial mass and the initial helium mass fraction (e.g. 500 0.80 0.248)
Each data are represented by 68 columns:
[1] Model number
[2] Maximum temperature Tmax (K)
[3] Mass coordinate of Tmax (Msun)
[4] Effective temperature Teff (K)
[5] Surface luminosity L (Lsun)
[6] Photospheric radius Reff (Rsun)
[7] Photospheric density rhoeff (g.cm-3)
[8] Density at the location of Tmax, rhomax (g.cm-3)
[9] Stellar mass M (Msun)
[10] Mass-loss rate (Msun.yr-1)
[11] Age t (yr)
[12] Photospheric gravity log(geff) (log(cgs))
[13] Central temperature Tc (K)
[14] Central pressure Pc
[15] Mass at the base of the convective envelope (Msun)
[16] Mass of the core (Msun)
Surface abundances
[17] H1
[18] H2
[19] He3
[20] He4
[21] Li6
[22] Li7
[23] Be7
[24] Be9
[25] B10
[26] B11
[27] C12
[28] C13
[29] C14
[30] N14
[31] N15
[32] O16
[33] O17
[34] O18
[35] F19
[36] Ne20
[37] Ne21
[38] Ne22
[39] Na23
[40] Mg24
[41] Mg25
[42] Mg26
[43] Al26m
[44] Al26g
[45] Al27
[46] Si28
Central abundances
[47] H1
[48] He3
[49] He4
[50] C12
[51] C13
[52] C14
[53] N14
[54] O16
[55] O17
[56] O18
[57] F19
[58] Ne20
[59] Ne21
[60] Ne22
[61] Na23
[62] Mg24
[63] Mg25
[64] Mg26
[65] Al26m
[66] Al26g
[67] Al27
[68] Si28
The number of the line represents the following points (if possible):
Number 101 -> Zero age main sequence
Number 211 -> Turn-off
Number 271 -> Base of the RGB
Number 291 -> RGB tip
Number 451 -> Base of the AGB
Number 500 -> Maximum of luminosity of the AGB