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Updated: Apr 22, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
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協調したポロイド磁場によるスケールの原星体ジェットの実験室での形成

B Albertazzi1, A Ciardi2, M Nakatsutsumi3

  • 1Laboratoire d'Utilisation des Lasers Intenses (LULI), École Polytechnique, CNRS, Commissariat à l'Energie atomique et aux énergies alternatives (CEA), Université Pierre et Marie Curie (UPMC), F-91128 Palaiseau, France. Institut National de la Recherche Scientifique-Energie, Matériaux, Télécommunications (INRS-EMT), Varennes, Québec, Canada. Graduate School of Engineering, Osaka University, Suita 565-0871, Japan.

Science (New York, N.Y.)
|October 18, 2014
PubMed
まとめ

実験室での実験では,ポロイド磁場は,天体物理学的ジェットを安定的にコリマートすることができることを示しています. この集中したプラズマの流れは衝撃を引き起こし,HH 154.のような若い恒星物体の流出の底部で観測されたX線放射を説明します.

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