A model of two-stream non-radial accretion for binary X-ray pulsars

Details A model of two-stream non-radial accretion for binary X-ray pulsars A model of two-stream non-radial accretion for binary X-ray pulsars

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..82..343l&link_type=abstract

Astrophysics and Space Science, vol. 82, no. 2, Mar. 1982, p. 343-361.

Astronomy and Astrophysics

Astronomy

24

Binary Stars, Pulsars, Stellar Mass Accretion, Stellar Models, X Ray Astronomy, Magnetospheres, Neutron Stars, Stellar Winds

Scientific paper

The general case of non-radial accretion is assumed to occur in real binary systems containing X-ray pulsars. The structure and the stability of the magnetosphere, the interaction between the magnetosphere and accreted matter, as well as evolution of neutron star in close binary system are examined within the framework of the two-stream model of nonradial accretion onto a magnetized neutron star. Observable parameters of X-ray pulsars are explained in terms of the model considered.

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