The tearing mode instability in accretion disc of neutron star and rapid X-ray burst

Details The tearing mode instability in accretion disc of neutron star and rapid X-ray burst The tearing mode instability in accretion disc of neutron star and rapid X-ray burst

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981scisn..24.1400w&link_type=abstract

Scientia Sinica, vol. 24, Oct. 1981, p. 1400-1405.

Astronomy and Astrophysics

Astronomy

4

Bursts, Magnetohydrodynamic Stability, Neutron Stars, Stellar Mass Accretion, Tearing Modes (Plasmas), X Ray Sources, Kepler Laws, Magnetic Field Configurations, X Ray Astronomy

Scientific paper

Tearing mode instability in the neutral sheet of a neutron star accretion disk is studied, where the plasma makes a Keplerian motion in the accretion disk and flows into the accretion disk continually from an outside source. The result is used to explain the burst mechanism of the rapid X-ray burst source MXB1730-335. The rise time of the burst, its energy, the time interval between two bursts, and the proportionality in the energy of consecutive bursts are fairly explained by the mechanism.

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