On the origin of the correlations between Gamma-Ray Burst observables
arXiv:astro-ph/0701031 · doi:10.1086/518305
Abstract
Several pairs of observable properties of Gamma Ray Bursts (GRBs) are known to be correlated. Many such correlations are straightforward predictions of the 'cannonball' model of GRBs. We extend our previous discussions of the subject to a wealth of new data, and to correlations between 'lag-time', 'variability' and 'minimum rise-time', with other observables. Schaefer's recent systematic analysis of the observations of many GRBs of known red-shift gives us a good and updated data-basis for our study.
Added Appendix. Accepted for publication in The Astrophysical Journal
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Cited by in corpus (19)
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