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Can GRB early X-ray afterglows be explained by a contribution from the reverse shock?

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

We propose to explain the recent observations of early X-ray afterglows by SWIFT from the dissipation of energy in the reverse shock sweeping back into the ejecta. We compute the evolution of the dissipated power and discuss the possibility that it can be radiated in the X-ray range.

Original languageEnglish
Title of host publicationGAMMA-RAY BURSTS IN THE SWIFT ERA
Subtitle of host publicationSixteenth Maryland Astrophysics Conference
Pages313-316
Number of pages4
DOIs
Publication statusPublished - 19 May 2006
Externally publishedYes
EventGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C., United States
Duration: 29 Nov 20052 Dec 2005

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
Country/TerritoryUnited States
CityWashington, D.C.
Period29/11/052/12/05

Keywords

  • Gamma-ray bursts
  • Gamma-ray sources
  • Shock waves

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