A model of the rapid burster |
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| Authors: | S Hayakawa |
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| Institution: | Department of Astrophysics, Nagoya University, Nagoya, Japan |
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| Abstract: | A new burst mode of MXB 1730 - 335, the rapid burster, as discovered by Hakucho in August 1979, is characterized by a train of long X-ray bursts whose behaviour is dictated by the accretion rate. In this mode the burst luminosity reaches the Eddington limit, so that the X-ray pressure controls the accretion from a reservoir in the magnetopause and accretion columns in the polar regions explain general features of the rapid burster observed in August 1979. |
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