The 4.5+/-0.5 soft gamma repeaters in review

Details The 4.5+/-0.5 soft gamma repeaters in review The 4.5+/-0.5 soft gamma repeaters in review

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..515h&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 515-522 (2000).

Computer Science

17

Gamma-Ray Sources, Gamma-Ray Bursts, Neutron Stars

Scientific paper

Four Soft Gamma Repeaters (SGRs) have now been identified with certainty, and a fifth has possibly been detected. I will review their X-ray and gamma-ray properties in both outburst and quiescence. The magnetar model accounts fairly well for the observations of SGR1806-20 and SGR1900+14, but data are still lacking for SGR1627-41 and SGR0525-66. The locations of the SGRs with respect to their supernova remnants suggest that they are high velocity objects. .

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