Early Hard X-ray Afterglows of Short GRBs with Konus Experiments
Astrophysics
2007-05-23 v1
Abstract
For a ten of 125 short GRBs observed by Konus-Wind and the Konus-A the existance of statistically significant flux of hard photons accompanying initial event for a time of tens to hundred seconds after the trigger was revealed. Temporal, spectral, and energetic characteristics of these events are presented. The statistical analysis of the whole burst sample reveals that the afterglow is a more common feature of short GRBs.
Keywords
Cite
@article{arxiv.astro-ph/0301318,
title = {Early Hard X-ray Afterglows of Short GRBs with Konus Experiments},
author = {D. D. Frederiks and R. L. Aptekar and S. V. Golenetskii and V. N. Il'inskii and E. P. Mazets and V. D. Palshin and T. L. Cline},
journal= {arXiv preprint arXiv:astro-ph/0301318},
year = {2007}
}
Comments
4 pages, 5 figures, talk at Rome 2002 GRB Conference