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Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter

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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 (Hardcover, 1985 ed.) Loot Price: R5,621
Discovery Miles 56 210
Mass Loss from Red Giants - Proceedings of a Conference held at the University of California at Los Angeles, U.S.A., June...

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 (Hardcover, 1985 ed.)

Mark Morris, Arie J. Zuckerman

Series: Astrophysics and Space Science Library, 117

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Loot Price R5,621 Discovery Miles 56 210 | Repayment Terms: R527 pm x 12*

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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?".

General

Imprint: Kluwer Academic Publishers
Country of origin: Netherlands
Series: Astrophysics and Space Science Library, 117
Release date: August 1985
First published: 1985
Editors: Mark Morris • Arie J. Zuckerman
Dimensions: 297 x 210 x 20mm (L x W x T)
Format: Hardcover
Pages: 320
Edition: 1985 ed.
ISBN-13: 978-90-277-2075-7
Categories: Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter > General
LSN: 90-277-2075-4
Barcode: 9789027720757

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