典型的なクワザール3C273の宇宙のダブルヘリックス
1Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany. alobanov@mpifr-bonn.mpg.de
まとめ
プラズマの不安定性の直接的な証拠は,ラジオ観測を用いた銀河外ジェットで発見された. ケルビン・ヘルムホルツの不安定性を示す二重螺旋構造は,クエーサー3C273ジェットで観測されました.
科学分野:
- 天体物理学 天体物理学
- プラズマ物理学 プラズマ物理学
背景:
- 活発な銀河核 (AGN) からの相対論的アウトフローを理解することは,天体物理学の鍵です.
- 銀河外ジェットにおけるプラズマの不安定性に関する直接的な証拠は,未だに難解である.
研究 の 目的:
- 銀河外ジェットにおけるプラズマの不安定性の直接的な証拠を見つけるために.
- AGN.からの相対論的アウトフローの性質を理解する.
主な方法:
- 軌道上のHALCA電波望遠鏡と地上望遠鏡を用いたラジオ干渉測定観測.
- クワザール3C273ジェットの高解像度画像.
主要な成果:
- ジェット全体で発生した放射は,二重の螺旋状構造を明らかにした.
- この構造は,ケルビン・ヘルムホルツ不安定性と一致しています.
- 軽量ジェット (ローレンツ因数2,マッハ数3.5) でモデル化された少なくとも5つの不安定モードを特定しました.
結論:
- 観測されたダブルヘリクスは,銀河外ジェットにおけるプラズマの不安定性の直接的な証拠を提供します.
- このモデルは,ジェットの内部構造と一般的な形状を正確に再現しています.
- この発見は,相対論的天体物理的アウトフローに関する私たちの理解を前進させます.
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