侧面左右
发表于 2025-3-26 23:51:04
CO Vibration Rotation Lines from Circumstellar Shells,a resolution of 3.5 km s., including CO lines from P(9) to R(14). In addition to the expected emission up to the expansion velocity of the envelope, both CO and .CO show evidence of high velocity features in the blue wing of the line, beyond the 15 km s. expansion velocity (Fig. 1).
贵族
发表于 2025-3-27 04:06:41
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Afflict
发表于 2025-3-27 05:23:12
0067-0057 more energy than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar
BRUNT
发表于 2025-3-27 12:27:35
Conference proceedings 1985y than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar to the stu
忧伤
发表于 2025-3-27 17:18:58
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爱花花儿愤怒
发表于 2025-3-27 19:45:59
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Urgency
发表于 2025-3-28 00:25:06
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accrete
发表于 2025-3-28 02:53:59
Mass Loss from Red Giants: Infrared Spectroscopy,ns have been made of 20 molecular species. CO is the most widely observed molecule and useful information has been gleaned from the observed rotational excitation, kinematics, time variability and spatial structure of the its lines. Examples of different observing techniques are discussed in the following sections.
foliage
发表于 2025-3-28 08:41:34
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Landlocked
发表于 2025-3-28 11:59:06
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