Titlebook: Mass Loss from Red Giants; Proceedings of a Con Mark Morris,Ben Zuckerman Conference proceedings 1985 D. Reidel Publishing Company, Dordrec

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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).

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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

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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

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Urgency

accrete

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.

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