宇宙 の 網 の 糸 で 二つ の 銀河 群 を 結ぶ ラジオ 脊
F Govoni1, E Orrù2, A Bonafede3,4,5
1Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Cagliari Via della Scienza 5, I09047 Selargius, Italy. federica.govoni@inaf.it.
まとめ
銀河団Abel 0399とAbel 0401の間の放射は 磁場と再加速した粒子を 含んだ光線を示唆しています LOFAR望遠鏡で観測されたこの現象は 弱い衝撃によるものかもしれません
科学分野:
- 宇宙学
- 天体物理学
- ラジオ天文学
背景:
- 銀河団は最大の重力結合構造です
- 銀河団が合体すると 銀河団内のガスに 衝撃と乱れが生じます
- 相対論的粒子と磁場は 宇宙構造の重要な構成要素です
研究 の 目的:
- 銀河団アベル0399とアベル0401を結ぶ 放射状の山脈を調査する
- クラスタ間フィラメントの相対性電子と磁場の起源を理解する.
- 銀河団の郊外で 粒子加速を繰り返す 衝撃の役割を探るため
主な方法:
- 低周波配列望遠鏡 (LOFAR) を用いて140MHzで放射を観測する.
- 2つの銀河団をつなぐラジオ放射の山脊の分析
- 粒子加速メカニズムをモデル化するための宇宙学的シミュレーション
主要な成果:
- アベール0399とアベール0401の間には 放射線が検出されました
- 放射は相対性電子と磁場の存在を示している.
- シミュレーションによると 弱い衝撃は 既存の相対性粒子に 反応を加速させます
結論:
- 観測された電波放射は,磁気フィラメント内の再加速された相対性粒子によって引き起こされる可能性があります.
- これらの粒子にエネルギーを与えるのは,体積全体に分散した弱い衝撃のせいかもしれません.
- この発見は 宇宙のウェブにおける 粒子加速の過程に光を当てます
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