Computation of convective model atmospheres of cool white dwarfs

Details Computation of convective model atmospheres of cool white dwarfs Computation of convective model atmospheres of cool white dwarfs

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.105...39g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 105, no. 1, Oct. 1984, p. 39-45.

Statistics

Computation

Atmospheric Models, Computational Astrophysics, Convection, Stellar Atmospheres, White Dwarf Stars, Computer Programs, Iteration, Stellar Temperature

Scientific paper

The results of test computations of strongly convective plane-parallel LTE models of white-dwarf atmospheres with Te = 5000 or 8000 K and log g = 8 are presented in a table and discussed. A longer iteration step is developed to stabilize the convective-zone boundary in one or two computations of the radiative-flux, which can then be omitted in a number of iterations, saving computation time without increasing the overall number of iterations required.

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