Testing the External Shock Model of Gamma-Ray Bursts using the Late-Time Simultaneous Optical and X-ray Afterglows
arXiv:0707.2826 · doi:10.1086/522930
Abstract
We study the ``normal'' decay phase of the X-ray afterglows of gamma-ray bursts (GRBs), which follows the shallow decay phase, using the events simultaneously observed in the R-band. The classical external shock model -- in which neither the delayed energy injection nor time-dependency of shock micro-physics is considered -- shows that the decay indices of the X-ray and R-band light curves, and , obey a certain relation, and that in particular, should be larger than -1/4 unless the ambient density increases with the distance from the central engine. For our selected 14 samples, we have found that 4 events violate the limit at more than the 3 level, so that a fraction of events are outliers of the classical external shock model at the ``normal'' decay phase.
Accepted for publication in ApJL. 12 page, 2 figures, 2 tables
References in corpus (11)
- A comprehensive analysis of Swift/XRT data: I. Apparent spectral evolution of GRB X-ray tails
- "Late prompt" emission in Gamma Ray Bursts?
- Hypernova Signatures in the Late Rebrightening of GRB 050525A
- Optical Photometry of GRB 021004: The First Month
- "Anomalous" Optical GRB Afterglows are Common: Two z~4 Bursts, GRB 060206 and 060210
- Optical and X-Ray Observations of GRB 060526: A Complex Afterglow Consistent with An Achromatic Jet Break
- RAPTOR observations of delayed explosive activity in the high-redshift gamma-ray burst GRB 060206
- The nature of the X-Ray Flash of August 24 2005
- Multi-color Shallow Decay and Chromatic Breaks in the GRB 050319 Optical Afterglow
- Extensive multiband study of the X-ray rich GRB 050408. A likely off-axis event with an intense energy injection
- A Unified Model of the Prompt Optical Emission of Gamma-Ray Bursts