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Swift XRT observations of X-ray flares in GRB afterglows

  • David N. Burrows
  • , P. Romano
  • , O. Godet
  • , A. Falcone
  • , C. Pagani
  • , G. Cusumano
  • , S. Campana
  • , G. Chincarini
  • , J. E. Hill
  • , P. Giommi
  • , M. R. Goad
  • , J. A. Kennea
  • , S. Kobayashi
  • , P. Mészáros
  • , J. A. Nousek
  • , J. P. Osborne
  • , P. T. O'Brien
  • , K. L. Page
  • , G. Tagliaferri
  • , B. Zhang

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

Abstract

The Swift XRT has been observing GRB afterglows since December 23, 2004. Three-quarters of these observations begin within 200 s of the burst onset, providing an unprecendented look at the behavior of X-ray emission from GRB afterglows in the first few hours after the burst. While most of the early afterglows have smoothly declining lightcurves, a substantial fraction has large X-ray flares on short time-scales. We suggest that these flares provide support for models with extended central engine activity producing late-time internal shocks.

Original languageEnglish (US)
Title of host publicationX-ray Universe 2005
Pages877-883
Number of pages7
Edition604
StatePublished - 2006
EventX-ray Universe 2005 - Madrid, Spain
Duration: Sep 26 2005Sep 30 2005

Publication series

NameEuropean Space Agency, (Special Publication) ESA SP
Number604
Volume2
ISSN (Print)0379-6566

Other

OtherX-ray Universe 2005
Country/TerritorySpain
CityMadrid
Period9/26/059/30/05

All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Space and Planetary Science

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