Stellar wind flow around an X-ray source

Details Stellar wind flow around an X-ray source Stellar wind flow around an X-ray source

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sval....3...64k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 3, Mar. 1977, p. 124-128.) Soviet Astronomy Letters, vol. 3, Mar.-Apr. 1977, p. 64-66.

Astronomy and Astrophysics

Astrophysics

3

Bow Waves, Plasma Heating, Shock Waves, Stellar Winds, X Ray Sources, Astrophysics, Binary Stars, Compton Effect, Stellar Mass Accretion

Scientific paper

The formation of a bow wave in front of an X-ray source, due to heating
of the stellar wind by its radiation is examined. A similar solution
describing the flow behind the source is obtained, assuming that the
Compton effect is the principal mechanism of plasma heating.

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