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Updated: Aug 13, 2026

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冲击激发的OH质光束辐射勾勒出银河系中心超新星残留物G359.1-0.05的轮

F Yusef-Zadeh1, K I Uchida, D Roberts

  • 1Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208, USA.

Science (New York, N.Y.)
|December 15, 1995
PubMed
概括

天文学家在银河系中心外 (G359.1-0.5) 附近检测到1720兆赫的扩展氧化 (OH) 质量辐射. 这一发现支持了这样一个理论:超新星残骸膨胀的冲击活动会触发OH质光线.

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