Kulkarni, S. R. and Berger, E. and Bloom, J. S. and Chaffee, F. and Diercks, A. and Djorgovski, S. G. and Frail, D. A. and Galama, T. J. and Goodrich, R. W. and Harrison, F. A. and Sari, R. and Yost, S. A. (2000) The afterglows of gamma-ray bursts. In: Gamma Ray Bursts: 5th Huntsville Symposium, Huntsville, AL, 18-22 October 1999. American Institute of Physics Conference Proceedings (526). American Institute of Physics , Melville, NY, pp. 277-297. ISBN 1-56396-947-5 http://resolver.caltech.edu/CaltechAUTHORS:KULaipcp00c
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:KULaipcp00c
Gamma-ray burst astronomy has undergone a revolution in the last three years, spurred by the discovery of fading long-wavelength counterparts. We now know that at least the long-duration GRBs lie at cosmological distances with estimated electromagnetic energy release of 10^51–10^53 erg, making these the brightest explosions in the Universe. In this article we review the current observational state, beginning with the statistics of X-ray, optical, and radio afterglow detections. We then discuss the insights these observations have given to the progenitor population, the energetics of the GRB events, and the physics of the afterglow emission. We focus particular attention on the evidence linking GRBs to the explosion of massive stars. Throughout, we identify remaining puzzles and uncertainties, and emphasize promising observational tools for addressing them. The imminent launch of HETE-2 and the increasingly sophisticated and coordinated ground-based and space-based observations have primed this field for fantastic growth.
|Item Type:||Book Section|
|Additional Information:||©2000 American Institute of Physics. Issue Date: September 8, 2000. Our research is supported by NASA and NSF. JSB holds a Fannie & John Hertz Foundation Fellowship, AD holds a Millikan Postdoctoral Fellowship in Experimental Physics, TJG holds a Fairchild Foundation Postdoctoral Fellowship in Observational Astronomy and RS holds Fairchild Foundation Senior Fellowship in Theoretical Astrophysics. The VLA is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The W.M. Keck Observatory is operated by the California Association for Research in Astronomy, a scientific partnership among California Institute of Technology, the University of California and the National Aeronautics and Space Administration. It was made possible by the generous financial support of the W.M. Keck Foundation.|
|Group:||Space Radiation Laboratory|
|Subject Keywords:||gamma-ray sources (astronomical), intergalactic matter, sky brightness, astronomical techniques, gamma-ray scattering, afterglows, cosmic ray energy spectra, astrophysical radiation mechanisms, X-ray astronomy|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Archive Administrator|
|Deposited On:||17 Dec 2007|
|Last Modified:||04 Mar 2013 18:51|
Repository Staff Only: item control page