Tail emission of prompt gamma-ray burst jets

Ryo Yamazaki, Kenji Toma, Kunihito Ioka, Takashi Nakamura

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Tail emission of the prompt gamma-ray burst is discussed using a multiple emitting sub-shell (inhomogeneous jet, sub-jets) model. The tail is a superposition of a number of smooth, long-duration, dim, and soft pulses emitted by segments located far from the line of sight. We find that the behavior of the tail is not so much affected by the local inhomogeneity but affected by the global sub-jet distribution. Some observed tails may disfavor the power-law jets.

Original languageEnglish
Title of host publicationGAMMA-RAY BURSTS IN THE SWIFT ERA
Subtitle of host publicationSixteenth Maryland Astrophysics Conference
Pages205-208
Number of pages4
DOIs
Publication statusPublished - 2006 May 19
Externally publishedYes
EventGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C., United States
Duration: 2005 Nov 292005 Dec 2

Publication series

NameAIP Conference Proceedings
Volume836
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference
CountryUnited States
CityWashington, D.C.
Period05/11/2905/12/2

Keywords

  • Gamma-ray burst

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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