GRB 060206 and the quandary of achromatic breaks in afterglow light curves

P. A. Curran, A. J. van der Horst, R. A.M.J. Wijers, R. L.C. Starling, A. J. Castro-Tirado, J. P.U. Fynbo, J. Gorosabel, A. S. Järvinen, D. Malesani, E. Rol, N. R. Tanvir, K. Wiersema, M. R. Burleigh, S. L. Casewell, P. D. Dobbie, S. Guziy, P. Jakobsson, M. Jelínek, P. Laursen, A. J. LevanC. G. Mundell, J. Näränen, S. Piranomonte

Research output: Contribution to journalLetter

26 Citations (Scopus)

Abstract

Gamma-ray burst afterglow observations in the Swift era have a perceived lack of achromatic jet breaks compared with the BeppoSAX era. We present our multi-wavelength analysis of GRB 060206 as an illustrative example of how inferences of jet breaks from optical and X-ray data might differ. The results of temporal and spectral analyses are compared, and attempts are made to fit the data within the context of the standard blast wave model. We find that while the break appears more pronounced in the optical and evidence for it from the X-ray alone is weak, the data are actually consistent with an achromatic break at about 16 h. This break and the light curves fit standard blast wave models, either as a jet break or as an injection break. As the pre-Swift sample of afterglows are dominated by optical observations, and in the Swift era most well-sampled light curves are in the X-ray, caution is needed when making a direct comparison between the two samples, and when making definite statements on the absence of achromatic breaks.

Original languageEnglish
Pages (from-to)L65-L69
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume381
Issue number1
DOIs
Publication statusPublished - 1 Oct 2007

Keywords

  • Gamma-rays: bursts
  • Radiation mechanisms: non-thermal
  • X-rays: individual: GRB 060206

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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