X-ray flares in the early swift observations of the possible naked burst GRB 050421

  • O. Godet
  • , K. L. Page
  • , M. R. Goad
  • , A. P. Beardmore
  • , P. T. O'Brien
  • , J. P. Osborne
  • , D. N. Burrows
  • , M. Capalbi
  • , J. Kennea
  • , V. Mangano
  • , A. Moretti
  • , D. Morris

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

Abstract

We present the Swift observations of the faint burst GRB 050421. The X-ray light-curve shows two flares: the first flare peaking at ∼ 110 s after the BAT trigger (T0) and the second one peaking at ∼154 s. We argue that the mechanism producing these flares is probably late internal shocks. The X-ray light-curve shows a rapid decline with a temporal index α ∼ 3.1. The X-ray source disappears completely less than 1 hour after the trigger. An X-ray spectral softening is also observed with time from β ∼ 0.1 to ∼ 1.2. A good joint fit to the BAT and XRT spectra indicates that the early X-ray and Gamma-ray emissions are produced by the same mechanism. The X-ray spectral softening is likely due to a shift down to lower energies of the peak of the prompt emission, and the rapid decline of the X-ray emission is probably the tail of the prompt emission. This suggests that the X-ray emission is completely dominated by high latitude radiation and the external shock, if any, is below the detection threshold.

Original languageEnglish (US)
Title of host publicationX-ray Universe 2005
Pages899-900
Number of pages2
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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