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Mass Loss in Metal Deficient Red Giants

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Mass Loss from Red Giants

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

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Abstract

The occurrence and rate of mass loss from metal deficient red giant field stars have consequences for the theory of evolution of low mass stars. This paper reports several of the results from an observational and theoretical program to assess the presence and character of chromospheric line profiles and their variations, to obtain quantitative measurements of radiative losses from chromospheres, and to construct semi-empirical model chromospheres and extended atmospheres in order to provide limits on the mass loss rates.

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Author information

Authors and Affiliations

  1. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA, 02138, USA

    A. K. Dupree, L. Hartmann, G. H. Smith & E. H. Avrett

Authors
  1. A. K. Dupree
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  2. L. Hartmann
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  3. G. H. Smith
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  4. E. H. Avrett
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Editor information

Editors and Affiliations

  1. Department of Astronomy, UCLA, Los Angeles, California, USA

    Mark Morris  & Ben Zuckerman  & 

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© 1985 D. Reidel Publishing Company

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Dupree, A.K., Hartmann, L., Smith, G.H., Avrett, E.H. (1985). Mass Loss in Metal Deficient Red Giants. In: Morris, M., Zuckerman, B. (eds) Mass Loss from Red Giants. Astrophysics and Space Science Library, vol 117. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5428-1_4

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  • DOI: https://doi.org/10.1007/978-94-009-5428-1_4

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8896-1

  • Online ISBN: 978-94-009-5428-1

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