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Cited by 311

The DOI matches its Crossref record; 12 of the 12 references it cites were found in a registry or an index.

Light Curves of Gamma‐Ray Burst Optical Flashes

Open access
Kobayashi, Shiho·2000·The Astrophysical Journal

Abstract

The standard model of gamma-ray burst (GRB) afterglows assumes that relativistically expanding material is decelerating as a result of interaction with the surrounding medium. The afterglows are well described by the synchrotron radiation from a forward shock, while the strong optical flash associated with GRB 990123 can be attributed to the emission from a reverse shock. We give a detailed study on the reverse shock emission. The full light curves are calculated for long and short GRB cases. We discuss the lack of the prompt optical detections by ROTSE for GRB 981121 and GRB 981223.

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Metadata

Authors
Kobayashi, S.
Venue
The Astrophysical Journal
Published
2000-12-20
Volume
545
Issue
2
Pages
807-812
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1740968810
Cited by
311
References
12
FWCI
5.93
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Light Curves of Gamma‐Ray Burst Optical Flashes. https://app.cochat.ai/papers/10.1086/317869
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Kobayashi, S. (2000). Light Curves of Gamma‐Ray Burst Optical Flashes. The Astrophysical Journal. https://doi.org/10.1086/317869

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