X-ray emission from Be star binaries

Details X-ray emission from Be star binaries X-ray emission from Be star binaries

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292..257a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 292, May 1, 1985, p. 257-259.

Astronomy and Astrophysics

Astronomy

29

B Stars, Neutron Stars, Stellar Flares, Stellar Mass Accretion, X Ray Binaries, X Ray Sources, Heao 1, Magellanic Clouds, X Ray Astronomy

Scientific paper

A model in which a neutron star in an eccentric inclined orbit around a
Be star passes through a ring of matter around the Be star has been used
to explain the recurrent flares of X-ray emission from these systems.
The optical emission during X-ray flares is due to partial absorption
and reprocessing of the X-rays in the ring.

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