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Updated: Apr 22, 2026

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在实验室中,通过对齐的极状磁场形成一个缩放的原星喷气

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
概括

实验室实验表明,一个极形磁场可以稳定地对天体物理喷气进行聚合. 这种聚焦的等离子体流产生了冲击,解释了在年轻恒星物体流出的基础上观察到的X射线辐射,如HH 154.

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