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Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters

Y. F. Huang
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Abstract

The popular fireball/blastwave model of classical gamma-ray bursts is applied to soft gamma-ray bursts. It is found that X-ray afterglows from strong events may be above their quiescent levels for 40 -- 400 seconds. Optical afterglows may also be detectable. By monitoring the three repeaters, we will have an ideal way to check the fireball/blastwave model.

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Y. F. Huang. 2005-02-22. Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters. https://arxiv.org/abs/astro-ph/0502452

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