Statistics – Computation
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...365..321s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 365, Dec. 10, 1990, p. 321-331.
Statistics
Computation
39
Ionized Gases, Radiative Transfer, Stellar Winds, Supergiant Stars, X Ray Binaries, Computational Astrophysics, Stellar Mass Accretion, Stellar Mass Ejection, Stellar Spectra, X Ray Spectra
Scientific paper
This paper presents calculations of the effect of changing X-ray ionization conditions on the radiative force experienced by the stellar wind material in a massive X-ray binary system. The radiative line force from the radiation field of the primary is parameterized in terms of the Castor et al. (1975) force multiplier. The results show that the line force decreases sharply, but in a nonlinear way, with increasing X-ray ionization. The dynamic consequences of this effect are discussed.
Kallman Timothy R.
Stevens Ian R.
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