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Author | Title | Accn# | Year | Item Type | Claims |
| 1 |
Morris, Mark |
Mass Loss from Red Giants |
I00253 |
1985 |
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| Title | Mass Loss from Red Giants : Proceedings of a Conference held at the University of California at Los Angeles, U.S.A., June 20???21, 1984 |
| Author(s) | Morris, Mark;Zuckerman, Arie J |
| Publication | Dordrecht, Springer Netherlands, 1985. |
| Description | XVI, 320 p : online resource |
| Abstract Note | Red giant and supergiant stars have long been favorites of professional 6 and amateur astronomers. These enormous stars emit up to 10 times 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 to the study of pre-main-sequence stars. For example, optical astronomy gives us a tantalizing glimpse of star forming regions but to really investi?? gate young stars and protostars requires infrared and radio astronomy. The same is true of post-main-sequence stars that are losing mass. Optical astronomers can measure the atomic component of winds from red giant stars that are undergoing mass loss at modest rates 6 (M $ 10- M9/yr.). But to see dust grains and molecules properly, 5 especially in stars with truly large mass loss rates, ~ 10- M9/yr, one requires IR and radio astronomy. As this stage of copious mass loss only lasts for ~105 years one might be tempted to ask, "who cares?" |
| ISBN,Price | 9789400954281 |
| Keyword(s) | 1. Astronomy, Observations and Techniques
2. Astronomy???Observations
3. EBOOK
4. EBOOK - SPRINGER
5. Observations, Astronomical
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| Item Type | eBook |
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