Highlights of the Rome Workshop on Gamma-Ray Bursts in the Afterglow Era
arXiv:astro-ph/9909026 · doi:10.1051/aas:1999372
Abstract
I review some of the highlights of the Rome Workshop on Gamma-Ray Bursts, and discuss some of the questions these results pose about the nature and origin of gamma-ray bursts.
8 pages, Proceedings of Gamma-Ray Bursts in the Afterglow Era, Nov. 1998, Rome, F. Frontera & L. Piro eds., A&A Suppl. Ser., in press
Cited by in corpus (12)
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- Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
- A Unified Jet Model of X-Ray Flashes, X-Ray-Rich Gamma-Ray Bursts, and Gamma-Ray Bursts: I. Power-Law-Shaped Universal and Top-Hat-Shaped Variable Opening-Angle Jet Models
- Astrophysical and Astrobiological Implications of Gamma-Ray Burst Properties
- Neutrino, Neutron, and Cosmic Ray Production in the External Shock Model of Gamma Ray Bursts
- The Number of Supernovae from Primordial Stars in the Universe
- The Importance of Off-Jet Relativistic Kinematics in Gamma-Ray Burst Jet Models
- Flash-Heating of Circumstellar Clouds by Gamma Ray Bursts
- The Decline of the Source Population of Gamma-Ray Bursts and Their Luminosity Function
- Implications of Recent Observational Discoveries for the Nature and Origin of Gamma-Ray Bursts
- Testing Gamma-Ray Burst Jet Structure with the Distribution of Gamma-Ray Energy Release
- Observations of Gamma-ray Bursts with ASTRO-H and Fermi