A magnetic explanation for the rapid burster

Details A magnetic explanation for the rapid burster A magnetic explanation for the rapid burster

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...68..333k&link_type=abstract

Space Science Reviews, Volume 68, Issue 1-4, pp. 333-334

Physics

X-Ray Binary Mxb 1730-335, Mhd Relaxation, Filament

Scientific paper

The observations of X-ray Type II bursts from the low-mass X-ray binary MXB 1730-335 can be explained by a particular form of magnetic gating in the presence of steady external accretion. The requirements are a strong magnetic field of the neutron star (7×1011 2×1012 gauss at the surface), rotational symmetry and alignment of the field axis with the axis of a steadily accreting disk to within 6°.

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