主要内容:
找Swift短暴的前兆,大约10%有。
前兆和暴本身没有很大的区别,有和没有前兆的暴之间也没什么区别。
精彩摘抄:
 |
一个例子 |
文章信息:
- · arXiv e-print (arXiv:1009.1385)
- · References in the Article
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Title: |
| Precursors of short gamma-ray bursts |
Authors: |
| Troja, Eleonora; Rosswog, Stephan; Gehrels, Neil |
Publication: |
| eprint arXiv:1009.1385 |
Publication Date: |
| 09/2010 |
Origin: |
| ARXIV |
Keywords: |
| Astrophysics - High Energy Astrophysical Phenomena |
Comment: |
| 8 pages, 2 figures, accepted for publication in The Astrophysical Journal |
Bibliographic Code: |
| 2010arXiv1009.1385T |
Abstract
We carried out a systematic search of precursors on the sample of short GRBs observed by Swift. We found that ~8-10% of short GRBs display such early episode of emission. One burst (GRB 090510) shows two precursor events, the former ~13 s and the latter ~0.5 s before the GRB. We did not find any substantial difference between the precursor and the main GRB emission, and between short GRBs with and without precursors. We discuss possible mechanisms to reproduce the observed precursor emission within the scenario of compact object mergers. The implications of our results on quantum gravity constraints are also discussed.
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