Reclassification of gamma-ray bursts based on their brightness distributions

Details Reclassification of gamma-ray bursts based on their brightness distributions Reclassification of gamma-ray bursts based on their brightness distributions

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002basi...30..445s&link_type=abstract

Bulletin of the Astronomical Society of India, Vol.30, p. 445-448

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Scientific paper

A reclassification of the cosmic gamma-ray bursts has been done into two distinct classes on the basis of their brightness distributions. While one (majority) class is found to be compatible with a homogeneous and monoluminosity source population with simple cosmological effects folded into the brightness distribution function, the other, smaller population is not consistent with such a scenario and may need a consideration of source evolutionary effects.

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