カラブ星雲からのガンマ線フレア
A A Abdo1, M Ackermann, M Ajello
1National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA.
まとめ
クラブ星雲は,2009年と2010年に2つの強力なガンマ線フレアを経験し,ペタ電子・ボルト電子の存在を示しました. これらのエネルギー的な出来事は,天体物理学的源における粒子の加速に関する現在の理論に挑戦します.
科学分野:
- 高エネルギー天体物理学
- 粒子物理学の素粒子物理学について
- 観測天文学は,観測による天文学である.
背景:
- クラブ星雲は,若い活気のあるパルサーによって動いています.
- パルサーは,高エネルギー放射線を放射することが知られている.
研究 の 目的:
- クラブ星雲から2つの異なるガンマ線フレアを記述し,分析する.
- これらのフレアの原因となる粒子の起源とエネルギーを調査する.
主な方法:
- フェルミ・ガンマ線宇宙望遠鏡のLarge Area Telescope (LAT) を使用してガンマ線フレアの検出.
- ガンマ線流の分析と爆発の持続時間.
主要な成果:
- 2009年2月 (16日) と2010年9月 (4日) に2つのガンマ線フレアが観測されました.
- フレアの間,ガンマ線流は4と6の因数で増加した.
- フレアは,コンパクトな領域 (<1.4 × 10−2) のペタ電子・ボルト電子からの放射を示唆する.
結論:
- 観測されたフレアは,離散的な天文学的源と関連付けられた最も高いエネルギーの粒子と関連付けられています.
- 極端なエネルギーは,粒子加速機構の既存のモデルに挑戦します.
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