On the "canonical behaviour" of the X-ray afterglows of the Gamma Ray Bursts observed with Swift's XRT
arXiv:astro-ph/0512196 · doi:10.1086/506606
Abstract
The "canonical behaviour" of the early X-ray afterglows of long-duration Gamma-Ray Bursts (GRBs) --observed by the X-Ray Telescope of the SWIFT satellite-- is precisely the one predicted by the Cannonball model of GRBs.
Accepted for publication in ApJL
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- Gamma-Ray Bursts in the Swift Era
- A unifying view of Gamma Ray Burst Afterglows
- Prior Emission Model for X-ray Plateau Phase of Gamma-Ray Burst Afterglows
- Pulse Width Evolution of Late Time X-rays Flares in GRBs: Evidence For Internal Shocks
- The diverse broad-band light-curves of Swift GRBs reproduced with the cannonball model
- On the origin of the correlations between Gamma-Ray Burst observables
- 'Jet breaks' and 'missing breaks' in the X-Ray afterglow of Gamma Ray Bursts
- Less noticeable shallow decay phase in early X-ray afterglows of GeV/TeV-detected gamma-ray bursts
- Probing the Structure of Gamma-Ray Burst Jets with Steep Decay Phase of their Early X-ray Afterglows
- Pulsar's kicks and Gamma-ray bursts
- The Cosmic-Ray Spectra: News on their Knees
- Long gamma-ray bursts without visible supernovae: a case study of redshift estimators and alleged novel objects
- Optical Behavior of GRB 061121 around its X-Ray Shallow Decay Phase
- Light Curves of Swift Gamma Ray Bursts