The rapid burster - A weakly magnetized neutron star

Details The rapid burster - A weakly magnetized neutron star The rapid burster - A weakly magnetized neutron star

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..920h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 15, 1989, p. 920-923.

Astronomy and Astrophysics

Astrophysics

11

Bursts, Neutron Stars, Stellar Mass Accretion, X Rays, Astronomical Models, Luminosity, Magnetohydrodynamic Stability, Pulsars, Stellar Magnetospheres

Scientific paper

The magnetic field of a neutron star involved in the rapid burster MXB
1730-335 is studied using a MHD instability model for type II bursts. It
is suggested that the magnetic field on the surface is about 10 to the
8th G. The radius of the magnetosphere is estimated to be about 10 km.
Observational evidence supporting this hypothesis is examined.

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