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比較的 電子 の 大 量 に 包まれ て いる 銀河 群
V Cuciti1,2, F de Gasperin3,4, M Brüggen3
1Hamburger Sternwarte, University of Hamburg, Hamburg, Germany. vcuciti@hs.uni-hamburg.de.
Nature
|September 28, 2022
まとめ
銀河団の相対性電子と磁場は 既知よりもずっと遠くに広がり 典型的なラジオハロを超えて 広大で薄弱なラジオ放出を生み出します
科学分野:
- 宇宙磁気
- 銀河団物理学
- 高エネルギー天体物理学
背景:
- 銀河団の中央には磁場と相対性電子があります
- 集束は磁場を増幅し,クラスタ内の気流を介して電子を再加速します.
- これらの電子は1-10 GeVのエネルギーから拡散したラジオハロ (約1 Mpc2) を生成します.
研究 の 目的:
- 銀河団における相対性電子と磁場の範囲を調査する.
- 既知のラジオハロを超えて拡散したラジオ放射を特徴づける.
主な方法:
- 4つの銀河団の観測を分析した.
- 中央のラジオハロと拡張された拡散領域の間の放射特性を比較した.
主要な成果:
- 4つの星団は 放射能の範囲をはるかに超えて 散らばった放射能を放出しています 放射能の範囲の30倍を占めているのです
- この広大な領域の放射性は,ラジオハロよりも約20倍低い.
結論:
- 相対論的電子と磁場は 銀河団に浸透し,これまで観測されたよりずっと大きなスケールで
- 銀河団の外部の物理的条件は ラジオハロ内の条件と大きく異なる.
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