The Accretion Flow by Magnetic Neutron Star

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

In the present paper, the author discusses generally the accretion flow in a stellar magnetosphere. The accretion flow confines in a magnetic channel, and the accreting gas is heated rapidly in the polar region of the neutron star within several stellar radii from the neutron star; the high temperature gas emits X rays. These results agree with the major features of the accretion flow by a magnetic neutron star.

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