繰り返し発生する高速電波の周りの乱れ環境における磁場逆転
Reshma Anna-Thomas1,2, Liam Connor3,4, Shi Dai5,6,7
1Department of Physics and Astronomy, West Virginia University, Morgantown, WV 26506, USA.
まとめ
繰り返されるFRBの観測は,源の近くに非常に変動する磁場を明らかにします. これはFRBが 渦巻磁気プラズマ画面を通して 伝播することを示唆しています 恐らく2進の伴星から
科学分野:
- 天体物理学
- ラジオ天文学
背景:
- FRBは 銀河系外からの 激しい短時間の電波の閃きです
- 極性FRBは高磁気環境から発生します
研究 の 目的:
- 17ヶ月間繰り返すFRB 20190520Bの環境を調査する.
- 観測されたファラデー回転の変動の原因を理解するために
主な方法:
- 繰り返し発生するFRB 20190520Bの長期監視
- ファラデー回転と脱極化を含むFRBの偏振特性に関する分析.
主要な成果:
- 信号の逆転を含むFRB 20190520Bの非常に変動するファラデー回転を観測した.
- FRBの脱極化が 1-3GHz以下で検出されました.
- 視界の磁場成分の変化として解釈する.
結論:
- FRBの環境には 渦巻く磁気性プラズマスクリーンがある
- この画面は,ソースから 10^-5 パーセックに位置する.
- この画面は FRB源のバイナリコンパニオンの 恒星風と一致しています
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