File Syntax and Content

• Files are named mMzZ[dD], where
• M is the star initial mass (in solar units),
• Z is the star initial metallicity (in mass fraction) and
• D is the optional value of the overshooting parameter ( d = D Hp wher Hp is the pressure scale height).




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• Four files are available for each computed star, namely
• file.hrd: containing HRD informations, i.e. from the first left column,
• the model number,
• the phase number (1 for PMS, 2 for MS, 3 for Post-MS, ...),
• the total surface luminosity (in solar units),
• the corresponding bolometric absolute magnitude,
• the radius at photosphere (in solar units),
• the total surface radius [at optical depth = 0.005] (R, in solar units),
• the effective temperature (in K),
• the volumic mass at photosphere (in cgs),
• the gravity at photosphere (in log10 of cgs),
• the total mass (M, in solar units) and
• the age (in yr).
• file.var1: containing various informations, i.e. from the first left column,
• the model number,
• the central temperature (in K),
• the central volumic mass (in cgs),
• the central degeneracy parameter value,
• the mass coordinate of the central burning core (in solar units),
• the radius coordinate of the central burning core (relative to the total radius),
• the total contribution of nuclear reactions to the global luminosity (relative to the surface luminosity),
• the total contribution of gravitation to the global luminosity (relative to the surface luminosity),
• the moment of inertia of the convective envelope (in units of total M*R**2) and
• the moment of inertia of the central radiative core (in units of total M*R**2).
• file.var2: containing other various informations, i.e. from the first left column,
• the model number,
• the mass coordinate of the first convective region from the center (in solar units),
• the radius coordinate of the first convective region from the center (relative to the total radius),
• the mass coordinate at the bottom of the convective envelope (in solar units),
• the radius coordinate at the bottom of the convective envelope (relative to the total radius),
• the temperature at the bottom of the convective envelope (in log10 of K) and
• the volumic mass at the bottom of the convective envelope (in log10 of cgs).
• file.xsurf: containing surface abundance informations, i.e. from the first left column,
• the model number,
• the surface mass fraction of 2H,
• the surface mass fraction of 3He,
• the surface mass fraction of 6Li,
• the surface mass fraction of 7Li,
• the surface mass fraction of 9Be,
• the surface mass fraction of 10B and
• the surface mass fraction of 11B.