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Energy injection in GRB afterglows: the cases of Swift GRBs 050401, 050801 and 050802

机译:GRB余量中的能量注入:SWIFT GRBS 050401,050801和050802的情况

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Swift very fast follow up observations of Gamma-Ray Bursts have allowed us to discover a new feature of GRB afterglows: a phase of shallow decay, usually attributed to energy injection in the burst ejecta, which can last for several thousands of seconds both in the X-ray and optical bands. Here I shall discuss this phase in the cases of Swift GRBs 050401, 050801 and 050802.
机译:SWIFT非常快速的跟进观察Gamma射线爆发的观察使我们能够发现GRB余辉的新功能:浅衰减的阶段,通常归因于爆裂喷射物中的能量注入,这可以持续数千秒X射线和光带。在这里,我将在SWIFT GRBS 050401,050801和050802的情况下讨论此阶段。

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