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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
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急速なラジオバーストに関連した密度の高い磁気プラズマ
Kiyoshi Masui1,2, Hsiu-Hsien Lin3, Jonathan Sievers4,5
1Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia V6T 1Z1, Canada.
Nature
|December 4, 2015
まとめ
急速無線電波 (FRB) は大きなファラデー回転を示し,源の近くの磁化を示しています. この発見はFRBの起源のマグネタルモデルを支持し,中性子星の合併シナリオと区別する.
科学分野:
- 天体物理学
- 宇宙学
- ラジオ天文学
背景:
- 急速無線爆発 (FRB) は,数ミリ秒間の超銀河間無線トランジエントです.
- これまでのFRBは 検出可能な線形偏振を欠いており ファラデーの回転測定を妨げていました
- FRBの分散測定は 宇宙的な距離を示唆しています
研究 の 目的:
- FRB110523のファラデー回転を調査する
- FRBの源環境と起源を決定する.
主な方法:
- FRB110523のアーカイブデータの分析
- 銀河系と銀河間分散の測定をモデル化する.
- 回転量と分散特性の評価
主要な成果:
- FRB110523で 重要なファラデー回転が検出されました
- FRB源の磁気化と分散の証拠がある
- 限られた源の赤偏移は最大0.5です.
結論:
- 観測された磁気化と散乱は マグネターのような若いエネルギー源を好みます
- これは古い中性子星の 合併を伴うモデルに 挑戦しています
- FRBの環境は 宿主銀河の内部で 密集している可能性が高い
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