Statistical study of evolution of gamma-ray bursts detected by APEX/PHOBOS and BATSE/COMPTON instruments

The new method of statistical studying of cosmic gamma-ray bursts is presented based on the averaging of time profiles. The comparison is done between bright and dim events: while no differences were found between average flux curves, the hardness ratios pointed out the effect of hardness/brightness...

Full description

Saved in:
Bibliographic Details
Published in:Advances in space research 1995-05, Vol.15 (5), p.131-134
Main Authors: Mitrofanov, I.G, Chernenko, A.M, Pozanenko, A.S, Fishman, G.J, Meegan, C.A, Briggs, M.S, Paciesas, W.S, Sagdeev, R.Z
Format: Article
Language:English
Subjects:
Astrophysics
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:The new method of statistical studying of cosmic gamma-ray bursts is presented based on the averaging of time profiles. The comparison is done between bright and dim events: while no differences were found between average flux curves, the hardness ratios pointed out the effect of hardness/brightness correlation.
ISSN:0273-1177
1879-1948
DOI:10.1016/0273-1177(94)00052-3