A model of rapid burster MXB 1730-335

Details A model of rapid burster MXB 1730-335 A model of rapid burster MXB 1730-335

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..92..143s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 92, no. 1, May 1983, p. 143-148.

Astronomy and Astrophysics

Astrophysics

5

Neutron Stars, Red Giant Stars, Stellar Mass Accretion, Stellar Models, Taylor Instability, X Ray Sources, Bursts, Electron Emission, Globular Clusters, Nebulae, Stellar Magnetic Fields

Scientific paper

A model of rapid burster MXB 1730-335, the source of type II X-ray burst is proposed, based on the Rayleigh-Taylor instability due to interaction of relativistic electrons produced by the rapid rotation of a highly magnetized neutron star, and the infalling accreted matter through the magnetic funnel at the poles. Conclusions are made that type II X-ray burster may be a constant source of cosmic rays and such a mechanism may be the progenitor of some forms of nebulae.

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