クラブ星雲から発する強力なガンマ線フレアの発見
M Tavani1, A Bulgarelli, V Vittorini
1Istituto Nazionale di Astrofisica-Istituto di Astrofisica Spaziale e Fisica Cosmica (INAF-IASF) Roma, via del Fosso del Cavaliere 100, 00133 Roma, Italy. pi.agile@iasf-roma.inaf.it
まとめ
超新星残骸であるクランブ星雲は,AGILE衛星によって検出された予期せぬガンマ線フレアを示した. これらの強力で短命なイベントは,星雲放射の既存のモデルに挑戦します.
科学分野:
- 高エネルギー天体物理学
- スーパーノヴァの残骸の残骸
- パルサー物理学 パルサー物理学
背景:
- パルサーで動いている"カニの星雲"は,安定した放射を放っていると考えられていた.
- 以前の観測は,ガンマ線出力の有意な変動を示さなかった.
研究 の 目的:
- カラブ星雲から強烈なガンマ線フレアが検出されたことを報告し,分析する.
- これらの一時的な出来事の起源と影響を調査する.
主な方法:
- AGILE衛星を使用したガンマ線フレア (100 MeV10 GeV) の検出.
- フレアフルスと時間スケールの分析.
- チャンドラとハッブルからの補完的なX線と光学データの議論.
主要な成果:
- 2010年9月と2007年10月に強いガンマ線フレアが観測されました.
- ガマ線流は,静止期と比較して,フレアの間に3倍に増加しました.
- フレアの特徴は,パルサーに近い起源を示唆しています.
結論:
- 観測されたフレアは,クランブ星雲からの星雲放射の標準モデルに異議を唱える.
- この発見により,素粒子加速を伴う新しいモデルが求められ,おそらくショック駆動のプラズマ波の乱れによるものです.
- 加速のための約1日間のタイムスケールが提案されています.
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