Gamma-ray burst afterglows
arXiv:astro-ph/0611774 · doi:10.1016/j.asr.2007.01.016
Abstract
Extended, fading emissions in multi-wavelength are observed following Gamma-ray bursts (GRBs). Recent broad-band observational campaigns led by the Swift Observatory reveal rich features of these GRB afterglows. Here we review the latest observational progress and discuss the theoretical implications for understanding the central engine, composition, and geometric configuration of GRB jets, as well as their interactions with the ambient medium.
References added, accepted for publication in Advances in Space Research
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Cited by in corpus (23)
- Dark Energy
- The First Survey of X-ray Flares from Gamma Ray Bursts Observed by Swift: Spectral Properties and Energetics
- Observational Constraints on Cosmological Models with the Updated Long Gamma-Ray Bursts
- A unifying view of Gamma Ray Burst Afterglows
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- Shallow decay phase of the early X-ray afterglow from the external shock in wind environment
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- Nuclear Criticality as a Contributor to Gamma Ray Burst Events