2011年6月20日
Detection of high-energy gamma-ray emission during the X-ray flaring activity in GRB 100728A
Astrophysical Journal Letters
- 巻
- 734
- 号
- 2
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1088/2041-8205/734/2/L27
We present the simultaneous Swift and Fermi observations of the bright GRB 100728A and its afterglow. The early X-ray emission is dominated by a vigorous flaring activity continuing until 1ks after the burst. In the same time interval, high-energy emission is significantly detected by the Fermi/Large Area Telescope. Marginal evidence ofGeV emission is observed up to later times. We discuss the broadband properties of this burst within both the internal and external shock scenarios, with a particular emphasis on the relation between X-ray flares, theGeV emission, and a continued long-duration central engine activity as their power source. © 2011. The American Astronomical Society. All rights reserved.
- リンク情報
- ID情報
-
- DOI : 10.1088/2041-8205/734/2/L27
- ISSN : 2041-8205
- ISSN : 2041-8213
- eISSN : 2041-8213
- ORCIDのPut Code : 77153105
- arXiv ID : arXiv:1104.5496
- SCOPUS ID : 79959483574
- BibTex Code : 2011ApJ...734L..27A