Non-isotropic angular distribution for very short-time gamma-ray bursts?

Details Non-isotropic angular distribution for very short-time gamma-ray bursts? Non-isotropic angular distribution for very short-time gamma-ray bursts?

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526...97c&link_type=abstract

GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 97-101 (2000).

Mathematics

Logic

1

Gamma-Ray Sources, Gamma-Ray Bursts, Observational Cosmology, Cosmic Rays

Scientific paper

While the bulk of the gamma-ray bursts (GRBs) are now believed to be from cosmological distances, the origin of very short-time GRBs is still not known. In the past, we have shown that GRBs with time duration less than 100 ms may form a separate class of GRBs based on the hardness and time distribution of these events. We also showed that the ln N-ln S distribution is consistent with the expectation of a quasi-Euclidean distribution of sources. In this letter, we report the study of the angular location of these GRBs that show a strong deviation from isotropy within the Galactic coordinates of +180°

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