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- W2949067752 abstract "Bright X-ray flares are routinely detected by the Swift satellite during the early afterglow of gamma-ray bursts, when the explosion ejecta drives a blast wave into the external medium. We suggest that the flares are produced as the reverse shock propagates into the tail of the ejecta. The ejecta is expected to contain a few dense shells formed at an earlier stage of the explosion. We show an example of how such dense shells form and describe how the reverse shock interacts with them. A new reflected shock is generated in this interaction, which produces a short-lived X-ray flare. The model provides a natural explanation for the main observed features of the X-ray flares – the fast rise, the steep power-law decline and the characteristic peak duration Δt/t ≃ 0.1–0.3." @default.
- W2949067752 created "2019-06-27" @default.
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- W2949067752 date "2017-09-12" @default.
- W2949067752 modified "2023-10-17" @default.
- W2949067752 title "X-ray flares from dense shells formed in gamma-ray burst explosions" @default.
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- W2949067752 doi "https://doi.org/10.1093/mnrasl/slx143" @default.
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