ガンマ線爆発の後の明るいX線フレアが輝く
D N Burrows1, P Romano, A Falcone
1Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802, USA. burrows@astro.psu.edu
まとめ
ガンマ線爆発 (GRB) の後光で検出された明るいX線フレアは,その中心的なエンジンは,最初の爆発の長時間後に活発に留まることを示唆しています. これらの発見は,長時間の活動期間と数百秒間の内部ショックを明らかにします.
科学分野:
- 天体物理学と宇宙学について
- 高エネルギー天体物理学
- 爆発的な天体物理現象
背景:
- ガンマ線爆発 (GRB) の余光は,大規模な爆発的な出来事とその中心的なエンジンについての洞察を提供します.
- 中央エンジンの活動期間と性質を理解することは,GRBの研究にとって極めて重要です.
研究 の 目的:
- GRBの余光の中で有意なX線フレアの発見を報告する.
- これらのフレアがGRBの中央エンジン活動に及ぼす影響を調査する.
主な方法:
- X線データを用いてGRBの余光の観測と分析.
- エネルギーとタイミングを含むX線フレア特性の特徴.
主要な成果:
- GRBの余光の中で2つの明るいX線フレアの発見.
- 1つの巨大なフレアは,GRBの総エネルギーで,GRBそのものに匹敵していた.
- これらのフレアは,最初のGRBイベントの数分後にピークに達しました.
結論:
- 観測されたX線フレアは,GRBにおける中央エンジンの活動が長期間続いたことを示している.
- 強い内部ショックは,ガンマ線放射後の数百秒間続く可能性が高い.
- GRBの中央エンジンは,長期にわたる強力な活動を示します.
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