Gamma-ray bursts and GRB080319B

Details Gamma-ray bursts and GRB080319B Gamma-ray bursts and GRB080319B

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spie.7502e..15m&link_type=abstract

Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2009. Edited by Romaniuk, Rys

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Gamma-Ray Bursts (GRB) are short impulses of gamma radiation (time duration ranges from 0.1 to 100 s) distributed almost isotropically across the sky. Most probably they arise during explosions or collisions of stars at cosmological distances. In this paper we discuss their origin, properties and current models. The methods of their observations will be also described. At the end short summary of "Pi of the Sky" GRBs observations will be presented, mainly focused on the naked-eye burst GRB080319B.

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