短时伽马射线暴的早期硬X射线尾后
天体物理学
2007-05-23 v1
摘要
对于125个由Konus-Wind和Konus-A观测到的10个短时伽马射线暴（short GRBs），发现在触发后持续数十到数百秒的硬色子通量具有统计学显著性。本文呈现了这些事件的时间、光谱和能量特征。整体样本的统计分析表明，尾后现象是短时伽马射线暴的更常见特征。
引用
@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}
}
备注
4 pages, 5 figures, talk at Rome 2002 GRB Conference