西瓜 发表于 2025-3-25 07:12:38

Mike Dean,Yuanbo Guo,Quan Z. Shengs thus exhibit their most violent surface activity during their PMS stage of evolution. Implications for the conditions in PMS stars, stellar activity-rotation age relation, for the chemistry and evolution of molecular clouds, and for various chemical and isotopic anomalies in the ancient solar syst

先驱 发表于 2025-3-25 10:10:25

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happiness 发表于 2025-3-25 14:16:53

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不透明 发表于 2025-3-25 16:45:50

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brachial-plexus 发表于 2025-3-25 20:05:35

X-ray emission from pre-main sequence stars,s thus exhibit their most violent surface activity during their PMS stage of evolution. Implications for the conditions in PMS stars, stellar activity-rotation age relation, for the chemistry and evolution of molecular clouds, and for various chemical and isotopic anomalies in the ancient solar syst

Temporal-Lobe 发表于 2025-3-26 02:32:36

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婴儿 发表于 2025-3-26 05:23:40

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去才蔑视 发表于 2025-3-26 12:26:54

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逢迎白雪 发表于 2025-3-26 14:15:21

Recent observations of T Tauri stars, chromosphere coronae, and extended envelopes which are often characterized by mass loss. Although some manifestations of T Tauri activity can be linked to vigorous solar-stellar phenomena characteristic of cool stars of low mass, other characteristics of T Tauri behavior are exhibited by a wide ran

主动脉 发表于 2025-3-26 17:47:27

X-ray emission from pre-main sequence stars,ncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof
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查看完整版本: Titlebook: Cool Stars, Stellar Systems, and the Sun; Proceedings of the T Sallie L. Baliunas,Lee Hartmann Conference proceedings 1984 Springer-Verlag