渐强
发表于 2025-3-23 13:04:59
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DAUNT
发表于 2025-3-23 15:15:48
Approximations Based on De Pril TransformsThe formation and evolution of massive (> 10M.) stars plays a key role in the final fate of their parental molecular clouds, and in the appearance and evolution of their host galaxies.
人类学家
发表于 2025-3-23 20:17:01
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expunge
发表于 2025-3-23 23:31:23
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范例
发表于 2025-3-24 03:46:35
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火车车轮
发表于 2025-3-24 07:32:32
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DNR215
发表于 2025-3-24 14:28:04
The Time-Series Estimation ProblemMost stars will experience episodes of substantial mass loss at some point in their lives. For very massive stars, mass loss dominates their evolution, although the mass loss rates are not known exactly, particularly once the star has left the main sequence.
Ovulation
发表于 2025-3-24 18:32:18
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Baffle
发表于 2025-3-24 20:20:42
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拥护
发表于 2025-3-25 00:59:53
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