X-ray bursts from magnetized accretion disks

Details X-ray bursts from magnetized accretion disks X-ray bursts from magnetized accretion disks

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...214..560w&link_type=abstract

Astrophysical Journal, Part 1, vol. 214, June 1, 1977, p. 560-565.

Astronomy and Astrophysics

Astronomy

27

Black Holes (Astronomy), Globular Clusters, Stellar Magnetic Fields, Stellar Mass Accretion, X Ray Sources, Bursts, Gamma Rays, Magnetohydrodynamic Waves, Stellar Mass, Stellar Models

Scientific paper

A model for the X-ray bursts of MXB 1730-335 and 3U 1820-30 (identified with the globular cluster NGC 6624) is presented in which a burst is due to the flarelike release of magnetic energy generated and stored as a toroidal field in an accretion disk. To fit the observed parameters, this model requires compact objects of the order of 10 solar masses, presumably black holes.

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