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Adiabatic Temperature Gradient White Dwarfs |
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The code given below generates models of white dwarfs in hydrostatic equilibrium with with an adiabatic temperature gradient for a general stellar equation of state. Such a model is useful for studying the simmering phase of white dwarf supernnova.
Temperature Profiles avaliable in pdf |
Energy Generation Profiles avaliable in pdf |
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adiabatic_white_dwarf_public.f plus four include files: implno.dek const.dek network.dek vector_eos.dek plus an eos data file: helm_table.dat |