GRB 160625Bの即時光学フラッシュ中の有意および可変の線形偏振
E Troja1,2, V M Lipunov3,4, C G Mundell5
1Department of Astronomy, University of Maryland, College Park, Maryland 20742-4111, USA.
Nature
|July 28, 2017
まとめ
ガンマ線爆発 (GRB) からの光学閃きで 顕著で変動する線形偏振を検出しました この発見は 中央のブラックホールに近い 相対論的ジェットの中の磁場構造の洞察を示しています
科学分野:
- 天体物理学
- 高エネルギー天体物理学
- ブラックホール物理学
背景:
- 恒星の質量を持つブラックホールは 相対論的なジェットを発射し,ガンマ線爆発 (GRB) を発生させます.
- これらのジェットの中の磁場を測定します
- 前回のGRBの二極化研究は,特に素早い放出段階では,議論の余地のある結果をもたらしました.
研究 の 目的:
- ガンマ線爆発 (GRB) のプロンプトフェーズ中の磁場構成を調査する.
- ポラライゼーションの性質を分析することで,素早いGRB放射の起源を理解する.
主な方法:
- GRB 160625Bに付随する瞬時の光学閃光の偏方測定観測.
- 素早く放出する段階における線形極化度と変動の分析.
主要な成果:
- プロンプト光学フラッシュで実質的な (8.3 ± 0.8%) 及び可変な線形偏振を検知する.
- 初期のジェット段階で ブラックホールの近くにある磁場構造を 探査しています
結論:
- 素早く冷却するシンクロトロン放射によって発生する.
- 大規模な磁場がブラックホールから噴出され 散布によって歪められ ジェットに浸透します
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