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
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…
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Produktdetails
Weitere Autoren: Zuckerman, Arie J. (Hrsg.)
- ISBN: 978-90-277-2075-7
- EAN: 9789027720757
- Produktnummer: 3430146
- Verlag: Springer Netherlands
- Sprache: Englisch
- Erscheinungsjahr: 1985
- Seitenangabe: 340 S.
- Masse: H26.0 cm x B18.3 cm x D2.3 cm 838 g
- Auflage: 1985
- Abbildungen: HC runder Rücken kaschiert
- Gewicht: 838
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