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Cited by 1,053

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Jets in Gamma-Ray Bursts

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Sari, Re'em, Piran, Tsvi, Halpern, J. P.·1999·The Astrophysical Journal

Abstract

In the afterglows of several gamma-ray bursts (GRBs), rapid temporal decay, which is inconsistent with spherical (isotropic) blast-wave models, is observed. In particular, GRB 980519 had the most rapidly fading of the well-documented GRB afterglows, with t -2.05±0.04 in optical as well as in X-rays. We show that such temporal decay is more consistent with the evolution of a jet after it slows down and spreads laterally, for which t - p decay is expected (where p is the index of the electron energy distribution). Such a beaming model would relax the energy requirements on some of the more extreme GRBs by a factor of several hundred. It is likely that a large fraction of the weak- (or no-) afterglow observations are also due to the common occurrence of beaming in GRBs and that their jets have already transitioned to the spreading phase before the first afterglow observations were made. With this interpretation, a universal value of p ≅ 2.4 is consistent with all data.

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Metadata

Authors
Sari, R., Piran, T., & Halpern, J. P.
Venue
The Astrophysical Journal
Published
1999-07-01
Volume
519
Issue
1
Pages
L17-L20
ISSN
0004-637X (ISSN-L)
OpenAlex
W1987204710
Cited by
1,053
References
1
FWCI
38.89
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Jets in Gamma-Ray Bursts. https://app.cochat.ai/papers/10.1086/312109
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Sari, R., Piran, T., & Halpern, J. P. (1999). Jets in Gamma-Ray Bursts. The Astrophysical Journal. https://doi.org/10.1086/312109

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