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Shallow Decay of Early X-Ray Afterglows from Inhomogeneous Gamma-Ray Burst Jets
Author(s) -
Kenji Toma,
Kunihito Ioka,
Ryo Yamazaki,
Takashi Nakamura
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/503384
Subject(s) - afterglow , gamma ray burst , physics , superposition principle , astrophysics , x ray , jet (fluid) , phase (matter) , light curve , satellite , astronomy , optics , mechanics , quantum mechanics
Almost all the X-ray afterglows of gamma-ray bursts (GRBs) observed by theSwift satellite have a shallow decay phase in the first thousands of seconds.We show that in an inhomogeneous jet (multiple-subjet or patchy-shell) modelthe superposition of the afterglows of off-axis subjets (patchy shells) canhave the shallow decay phase. The necessary condition for obtaining the shallowdecay phase is that gamma-ray bright subjets (patchy shells) should havegamma-ray efficiency higher than previously estimated, and should be surroundedby gamma-ray dim subjets (patchy shells) with low gamma-ray efficiency. Ourmodel predicts that events with dim prompt emission have the conventionalafterglow light curve without the shallow decay phase like GRB 050416A.Comment: 4 pages, 2 figures, accepted for publication in ApJ

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