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The Astrophysical Journal
Article . 2001 . Peer-reviewed
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https://dx.doi.org/10.1086/318...
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Generic Difference between Early and Late Stages of BATSE Gamma‐Ray Bursts

descriptionPublicationkeyboard_double_arrow_right Article 20 Jan 2001 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 547, pages 334-337 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Igor G. Mitrofanov; Maxim L. Litvak; Dmitrij S. Anfimov; Anton B. Sanin; Michael S. Briggs; William S. Paciesas; Geoffrey N. Pendleton; +2 Authors

doi: 10.1086/318347

Generic Difference between Early and Late Stages of BATSE Gamma‐Ray Bursts

Abstract

The early and late stages of gamma-ray bursts are studied in a statistical analysis of the large sample of long BATSE events. The primary peak is used as the boundary between the early and late stages of emission. Significant differences are found between the stages: the early stage is shorter, it has harder emission, and it becomes a smaller fraction of the total burst duration for burst groups of decreasing intensity.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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