Comparison of spherically symmetric and plane-parallel NLTE model stellar atmospheres

Details Comparison of spherically symmetric and plane-parallel NLTE model stellar atmospheres Comparison of spherically symmetric and plane-parallel NLTE model stellar atmospheres

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ppib.conf..125k&link_type=abstract

Physical Processe in Interacting Binaries, proceedings of the 19th Stellar Conference of the Slovak and Czech Astronomical Insti

Astronomy and Astrophysics

Astronomy

Stellar Atmospheres, Sphericity Effects

Scientific paper

The differences between equations for spherically symmetric and plane parallel static model atmospheres are summarized. Results of comparison of spherically symmetric and plane parallel static model atmospheres of hot stars are discussed for sample models of O stars, B stars, central stars of planetary nebulae, and white dwarfs. In general, the temperature of spherically symmetric models is lower in the outer layers, the continuum flux in the peak of intensity is lower, and lower members of line series are deeper.

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