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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

  • Conference proceedings
  • © 1985

Overview

Part of the book series: Astrophysics and Space Science Library (ASSL, volume 117)

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Table of contents (48 papers)

Keywords

About this book

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?".

Editors and Affiliations

  • Department of Astronomy, UCLA, Los Angeles, USA

    Mark Morris, Ben Zuckerman

Bibliographic Information

  • Book Title: Mass Loss from Red Giants

  • Book Subtitle: Proceedings of a Conference held at the University of California at Los Angeles, U.S.A., June 20–21, 1984

  • Editors: Mark Morris, Ben Zuckerman

  • Series Title: Astrophysics and Space Science Library

  • DOI: https://doi.org/10.1007/978-94-009-5428-1

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: D. Reidel Publishing Company, Dordrecht, Holland 1985

  • Hardcover ISBN: 978-90-277-2075-7Published: 31 August 1985

  • Softcover ISBN: 978-94-010-8896-1Published: 02 October 2011

  • eBook ISBN: 978-94-009-5428-1Published: 06 December 2012

  • Series ISSN: 0067-0057

  • Series E-ISSN: 2214-7985

  • Edition Number: 1

  • Number of Pages: XVI, 320

  • Topics: Astronomy, Observations and Techniques

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