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Prog. Theor. Phys. Vol. 56 No. 6 (1976) pp. 1772-1780
Binary Star Model for Recurrent X-Ray Bursts
Reiun Hōshi
Department of Physics, Rikkyo University, Tokyo 171
(Received July 2, 1976)
Abstract:
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.
URL :
http://ptp.ipap.jp/link?PTP/56/1772/
DOI : 10.1143/PTP.56.1772
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