autoantibodies
发表于 2025-3-21 19:57:21
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食品室
发表于 2025-3-21 20:52:50
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不自然
发表于 2025-3-22 00:39:53
Book 1981related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti cal developments on the problem of mass loss from early ty pe st
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发表于 2025-3-22 08:18:08
Summary, Conclusions, and Future Work,the WR mass loss may also be important for Of stars (Lamers 1980). A determination of the properties of the WR stellar winds will provide diagnostics which might aid in identifying the mass loss mechanism, and P-Cygni profiles form one important data source for this purpose. With the advent of IUE m
帽子
发表于 2025-3-22 12:38:46
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天气
发表于 2025-3-22 15:56:36
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天气
发表于 2025-3-22 20:25:06
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烧瓶
发表于 2025-3-23 00:08:49
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capsaicin
发表于 2025-3-23 03:25:34
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theta-waves
发表于 2025-3-23 07:50:55
An Introduction to Data Mining,± 100 km s.. Our preliminary evaluation of the associated mass loss rate gives 10. M. yr.. Other planetary nebulae nuclei are studied with low resolution IUE spectra and indications are found of mass loss rates consistent with the above value.