Clique
发表于 2025-3-21 17:56:37
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上下倒置
发表于 2025-3-22 00:17:00
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裤子
发表于 2025-3-22 01:08:14
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galley
发表于 2025-3-22 05:27:16
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Cosmopolitan
发表于 2025-3-22 09:19:09
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刺耳
发表于 2025-3-22 13:31:51
Ahmet Oğuz Akçay,Mehmet Arif Bozan velocities to −1380 and −1000 km s. respectively. In contrast, the absorptions are narrower with steeper wings in ζ Oph and υ Ori. The latter star also has emission, while in Oph the absorption is split into two components from about −1550 to −1280 and −1280 to −980 km s..
Ambulatory
发表于 2025-3-22 17:41:07
Ayşegül Oğuz Namdar,Bahadır Namdar,Fulden Guler Nalbantoglubefore making this choice. It is necessary to observe individual objects over extended periods of time at high dispersion to establish whether or not all WR’s are binary systems. It is also required firmly to establish the temporal nature of the variations, since short term periodicities would tend
善辩
发表于 2025-3-22 23:05:01
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背信
发表于 2025-3-23 01:50:24
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DUST
发表于 2025-3-23 06:34:21
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