抄録
GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.
本文言語 | English |
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ホスト出版物のタイトル | Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference |
ページ | 158-161 |
ページ数 | 4 |
巻 | 1000 |
DOI | |
出版ステータス | Published - 2008 |
外部発表 | はい |
イベント | Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM 継続期間: 2007 11 5 → 2007 11 9 |
Other
Other | Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 |
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City | Santa Fe, NM |
Period | 07/11/5 → 07/11/9 |
ASJC Scopus subject areas
- Physics and Astronomy(all)