Ligament
发表于 2025-3-25 03:45:27
ed with non-LTE WR model flux distributions. Comparisons of stellar effective temperatures and luminosities derived using this technique with those determined by modelling stellar emission lines can identify deficiencies such as the lack of line-blanketing in WR model atmospheres. Very hot WR stars
MENT
发表于 2025-3-25 11:30:43
http://reply.papertrans.cn/71/7023/702293/702293_22.png
无政府主义者
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多产鱼
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隐藏
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antecedence
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pacifist
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countenance
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嫌恶
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