The basic structure of hot white dwarfs atmospheres as a function of composition

Details The basic structure of hot white dwarfs atmospheres as a function of composition The basic structure of hot white dwarfs atmospheres as a function of composition

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....87..307b&link_type=abstract

Astronomy and Astrophysics, vol. 87, no. 3, July 1980, p. 307-314.

Astronomy and Astrophysics

Astrophysics

7

Chemical Composition, Far Ultraviolet Radiation, Radiant Flux Density, Stellar Atmospheres, White Dwarf Stars, Absorptivity, Abundance, Electron Scattering, Monochromatic Radiation, Nebulae, Stellar Models, Stellar Radiation, X Ray Sources

Scientific paper

Nongray model atmospheres and continuum surface flux distributions for hot white dwarfs have been calculated using seven different chemical compositions. These include typical DA, non-DA, HZ21, and HZ34 mixtures and (for comparison purposes) normal population I abundances. The results are used to obtain a better qualitative and intuitive understanding of the properties of hot white dwarf atmospheres and their dependence on chemical composition.

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