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arXiv · astro-ph/9912061

The 4.5 +/- 0.5 Soft Gamma Repeaters in Review

K. Hurley
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Abstract

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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K. Hurley. 1999-12-03. The 4.5 +/- 0.5 Soft Gamma Repeaters in Review. https://doi.org/10.1063/1.1361637

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