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現在の恒星形成と関連のない短いガンマ線爆発の起源です
S D Barthelmy1, G Chincarini, D N Burrows
1NASA/Goddard Space Flight Center Greenbelt, Maryland 20771, USA. scott@lheamail.gsfc.nasa.gov
Nature
|December 16, 2005
まとめ
短いガンマ線爆発 (GRB) は超新星から発生するものではありません. 新しい証拠によると,これらの宇宙爆発は,ニュートロン星やブラックホール-ニュートロン星バイナリの融合から発生している可能性が高い.
科学分野:
- 天体物理学 天体物理学
- 宇宙の爆発,宇宙の爆発.
- 高エネルギー天文学 高エネルギー天文学
背景:
- 検出された後光を持つ2つの短いガンマ線爆発 (GRB) は,宿主銀河の起源が不明でした.
- 一つの短いGRBは,星を形成する矮星銀河で,もう一つは,おそらく円銀河で発生しました.
研究 の 目的:
- 短ガンマ線爆発 (GRB) の起源を特定するために.
- 宿主銀河の性質と短いGRBの祖先系を調査する.
主な方法:
- 短いGRB 050724.4のX線位置づけ
- ガンマ線とX線の後発光特性に関する分析.
- 以前のGRB観測と理論モデルとの比較.
主要な成果:
- GRB 050724のX線余光は,赤道偏移 z = 0.258.8で円銀河の中心部から離れている位置に位置付けられました.
- 円銀河の恒星形成率が低いため,GRB 050724.4の超新星起源はありそうにない.
- 短いGRBは,長いGRBよりも著しく低い同位体エネルギーを示します.
結論:
- 短いGRBは,超新星爆発から発生する可能性は低い.
- 二重中性子星の合体または中性子星とブラックホールのペアは,短いGRBの祖先である可能性が高い.
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