Binary Star Model for Recurrent X-Ray Bursts

Details Binary Star Model for Recurrent X-Ray Bursts Binary Star Model for Recurrent X-Ray Bursts

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pthph..56.1772h&link_type=abstract

Progress of Theoretical Physics, Vol. 56, No. 6, pp. 1772-1780

Physics

Scientific paper

A model for the recurrent X-ray bursts from 3U1820-30 in the globular
cluster NGC 6624 is presented. The X-ray bursts are explained in terms
of instantaneous accretion by a compact binary companion when it
intersects an accretion disk surrounding a more massive black hole.

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