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27 April 2024
 
  » arxiv » astro-ph/0504331

 Article overview



Swift observations of GRB050128: the early X-ray afterglow
S. Campana ; L.A. Antonelli ; G. Chincarini ; S. Covino ; G. Cusumano ; D. Malesani ; V. Mangano ; A. Moretti ; C. Pagani ; P. Romano ; G. Tagliaferri ; M. Capalbi ; M. Perri ; P. Giommi ; L. Angelini ; P. Boyd ; D.N. Burrows ; J.E. Hill ; C. Gronwall ; J.A. Kennea ; S. Kobayashi ; P. Kumar ; P. Meszaros ; J.A. Nousek ; P.W.A. Roming ; B. Zhang ; A.F. Abbey ; A.P. Beardmore ; A. Breeveld ; M.R. Goad ; O. Godet ; K.O. Mason ; J.P. Osborne ; K.L. Page ; T. Poole ; N. Gehrels ;
Date 14 Apr 2005
Journal Astrophys.J. 625 (2005) L23-L26
Subject astro-ph
AbstractSwift discovered GRB050128 with the Burst Alert Telescope and promptly pointed its narrow field instruments to monitor the afterglow. X-ray observations started 108 s after the trigger time. The early decay of the afterglow is relatively flat with a temporal decay modeled with a power law with index ~ -0.3. A steepening occurs at later times (~ 1500 s) with a power law index of ~ -1.3. During this transition, the observed X-ray spectrum does not change. We interpret this behaviour as either an early jet break or evidence for a transition from the fast cooling regime to the slow cooling regime in a wind environment.
Source arXiv, astro-ph/0504331
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