Further Study of the Gamma-Ray Bursts Duration Distribution

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dc.creatorHorvath, I.
dc.date2002-05-01
dc.date.accessioned2026-07-07T06:22:10Z
dc.date.available2026-07-07T06:22:10Z
dc.descriptionTwo classes of gamma-ray bursts have been identified so far, characterized by durations shorter and longer than approximately 2 seconds. In 1998 two independent papers indicated the existence of the third class of the bursts roughly duration between 2 and 10 seconds. In this paper, using the full BATSE Catalog, the maximum likelihood estimation is presented, which gives a 0.5% probability to having only two subclasses. The Monte-Carlo simulation confirms this probability, too.
dc.descriptionsubmitted to A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0205004
dc.identifierhttp://arxiv.org/abs/astro-ph/0205004
dc.identifierAstron.Astrophys. 392 (2002) 791-793
dc.identifierdoi:10.1051/0004-6361:20020808
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95830
dc.subjectAstrophysics
dc.titleFurther Study of the Gamma-Ray Bursts Duration Distribution
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