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銀河中心の山脊から非常に高エネルギーのガンマ線を発見した
F Aharonian1, A G Akhperjanian, A R Bazer-Bachi
1Max-Planck Institut für Kernphysik, PO Box 103980, D 69029 Heidelberg, Germany.
Nature
|February 10, 2006
まとめ
銀河系宇宙線は,超新星残骸から発生する. 観測により,分子雲に関連した非常に高エネルギーガンマ線放射が明らかになり,陽子と原子核が源であることを示唆しています.
科学分野:
- 天体物理学 天体物理学
- 高エネルギー天文学 高エネルギー天文学
- 宇宙線物理学 宇宙線物理学
背景:
- 銀河系宇宙線 (最大10^15 eV) の起源は完全に理解されていません.
- 超新星残骸は,仮説的な源であり,ガンマ線観測は,宇宙線加速と拡散の研究の鍵となる.
研究 の 目的:
- 銀河系宇宙線の源を調査する.
- 銀河系の中央部の非常に高エネルギーガンマ線放射を分析するために.
主な方法:
- 拡張された非常に高エネルギー (> 10^11 eV) のガンマ線放射の観測.
- 銀河中心の巨大分子雲 (200パーセク) との空間的相関分析.
主要な成果:
- 超高エネルギーガンマ線放射の広大な領域が検出されました.
- この放射は,巨大な分子雲の複合体と空間的に相関しています.
- ガンマ線スペクトルの硬さは,宇宙線が電子ではなく,陽子や原子核であることを示唆しています.
結論:
- 観測されたガンマ線放射は,分子雲内の宇宙線相互作用から発生している可能性が高い.
- これらの宇宙線のエネルギー源は,およそ10^4年前の単一の超新星爆発かもしれません.
- この研究は,超新星残骸が銀河宇宙線の加速器であることを支持する証拠を提供します.
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