%%% old files without PHASE field. 
%%% These files are slightly different from the new ones, because they 
%%% have not been processed by the automatic isochrone machine

PARSEC V1.2s tracks

Bressan A. et al. 2012, MNRAS, 427, 127 (V1.1)

Chen Y. et al. 2014, MNRAS, 444, 2525  (very low mass stars down to 0.1 Msun)
Tang J. et al. 2014, arXiv:1410.1745   (massive stars up to ~ 350Msun or more)
Chen Y. et al. 2014, to be submitted   (new bolometric corrections for massive stars)


From pre main sequence to   
- 30Gyr very low mass stars
- He flash   low mass stars
- a few thermal pulses intermediate mass stars
- C ignition massive stars

HB evolution  of low mass stars


Small data tables containing

MODELL MASS AGE 
LOG_L LOG_TE LOG_R (log10 Luminosity Teff Radius)
LOG_RAT (mass loss rate if not zero)
M_CORE_HE  (mass of H exhausted core  -M_sun-) 
M_CORE_C   (mass of He exhausted core  -M_sun-) 
H_CEN   HE_CEN  C_cen  O_cen (central composition by mass)
LX LY LC LNEUTR L_GRAV (in L/Ltot)
H_SUP  HE_SUP  C_SUP  N_SUP  O_SUP (surface composition by mass)