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Updated: Jul 11, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
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在星爆星系M82中,热等离子体和黑洞二进制星系

R E Griffiths1, A Ptak, E D Feigelson

  • 1Department of Physics, Wean Hall, Carnegie Mellon University, Pittsburgh, PA 15213-3890, USA. griffith@astro.phys.cmu.edu

Science (New York, N.Y.)
|November 18, 2000
PubMed
概括

钱德拉X射线天文台的数据显示,Messier 82 (M82) 具有极其热的等离子体,由超新星驱动,为银河系风提供动力. 这项研究确定了紧的X射线源,可能是黑洞系统.

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