X-ray emission from certain nebulae formed by stellar wind

Details X-ray emission from certain nebulae formed by stellar wind X-ray emission from certain nebulae formed by stellar wind

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..274b&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 274-292. In Russian.

Astronomy and Astrophysics

Astronomy

5

Nebulae, Stellar Radiation, Stellar Spectra, Stellar Winds, X Ray Spectra, Gas Dynamics, Gas Ionization, Stellar Models, Temperature Distribution, X Ray Astronomy

Scientific paper

The fluxes and spectra of soft (0.1-4 keV) X-ray emission are calculated for six nebulae around stars with strong stellar winds: NGC 6888, S 119, S 308, NGC 2359, NGC 3199, and NGC 7635. Calculations are performed taking into account: (1) exact distributions of temperature and gas density for the gasdynamic model of Castor et al. (1975) and Weaver et al. (1977); and (2) deviations from the equilibrium gas ionization of the nebula.

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