シンビオティックバイナリ星 V407 Cygni のノヴァと同時進行するガンマ線放射
1, A A Abdo, M Ackermann
1Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA.
まとめ
天文学者は,新星V407 Cygniから予期せぬガンマ線放射を検出し,以前のモデルに挑戦しました. このノヴァは,新星です.
科学分野:
- 天体物理学 天体物理学
- 高エネルギー天体物理学
- 恒星の進化について
背景:
- ノバは,白矮星の増殖による恒星爆発である.
- 新星殻からX線放射が予想されますが,より高いエネルギーの放射はそうではありません.
- V407 Cygniは,最近光学新星が発生したシンビオティックな星系です.
研究 の 目的:
- ノバV407 Cygniからのガンマ線放射の検出を報告する.
- この予期せぬ高エネルギー放射の起源を調査する.
主な方法:
- フェルミ大望遠鏡による観測.
- 変数ガンマ線放射の分析 (0.1から10GeV).
主要な成果:
- V407 Cygni.からの変数ガンマ線放射の検出.
- 放射は0.1から10GeVのエネルギーに及ぶ.
結論:
- 提案されたメカニズム:新星殻と赤い巨人の密集した媒体の相互作用により,粒子が加速する.
- 陽子対陽子の相互作用は,pi(0) 崩壊ガンマ線を生成する可能性があります.
- 赤巨人の放射の逆コンプトン散乱は,確証されていないものの,放射源の可能性がある.
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