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• W2034352875 abstract "Soft X-ray flares were detected following the short-duration gamma-ray burst GRB 050724. The temporal properties of the flares suggest that they are likely due to the late-time activity of the central engine. We argue that if short GRBs are generated through compact star mergers, as is supported by the recent observations, the jet powering the late X-ray flares must be launched via magnetic processes rather than via neutrino-antineutrino annihilations. As a result, the X-ray flares following short GRBs are expected to be linearly polarized. The argument may also apply to the X-ray flares following long GRBs. Future observations with the upcoming X-ray polarimeters will test this prediction." @default.
• W2034352875 created "2016-06-24" @default.
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• W2034352875 date "2005-12-06" @default.
• W2034352875 modified "2023-09-23" @default.
• W2034352875 title "Linearly Polarized X-Ray Flares following Short Gamma-Ray Bursts" @default.
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• W2034352875 doi "https://doi.org/10.1086/499489" @default.
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