Testing models of the Soft Gamma Repeaters

Details Testing models of the Soft Gamma Repeaters Testing models of the Soft Gamma Repeaters

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..944t&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 944-946 (1998).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, Late Stages Of Stellar Evolution

Scientific paper

Models of the Soft Gamma Repeater sources involve two key parameters: magnetic field strength and rotation period. Several relevant observational probes of the SGRs are discussed, including: their quiescent X-ray and particle emission; the X-ray afterglow from the heated surface of the neutron star following a burst; and an anomalous group of low luminosity X-ray pulsars with properties very similar to SGR 0526-66 in its quiescent state (the best studied of which is 1E2259+586) [19,5].

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