Balazs 2009 光学亮暴和暗暴在伽玛和X射线的表现是有区别的
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· Find Similar Abstracts (with default settings below) - · arXiv e-print (arXiv:0903.5275)
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Title: | Observational difference between gamma and X-ray properties of optically dark and bright GRBs | |
Authors: | Balazs, L. G.; Horvath, I.; Bagoly, Z.; Meszaros, A.; Veres, P. | |
Publication: | eprint arXiv:0903.5275 | |
Publication Date: | 03/2009 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena | |
Comment: | Santa Fe proc | |
Bibliographic Code: | 2009arXiv0903.5275B |
Abstract
Using the discriminant analysis of the multivariate statistical analysis we compared the distribution of the physical quantities of the optically dark and bright GRBs, detected by the BAT and XRT on board of the Swift Satellite. We found that the GRBs having detected optical transients (OT) have systematically higher peak fluxes and lower HI column densities than those without OT.Bibtex entry for this abstract Preferred format for this abstract (see Preferences)
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