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Better determinations of mass loss rates for red giants and supergiants

  • Stephen A. Drake
  • Jeffrey L. Linsky
6. Workshop on Alpha Orionis
Part of the Lecture Notes in Physics book series (LNP, volume 193)

Keywords

Mass Loss Rate Stellar Wind Will Emit Chromospheric Emission Luminous Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Aldrovandi S.M.V., Péquignot D., Astron. Astrophys. 25, 321 (1973)Google Scholar
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  4. Jordan C., Brown A., in Solar Phenomena in Stars and Stellar Systems, Proceedings of NATO Advanced Study Institute, Bonas, p.199, pub. D. Reidel, 1980Google Scholar
  5. Stencel R.E., Linsky J.L., Brown A., Jordan C., Carpenter K.G., Wing R.F., Czyzak S., MNRAS 195 27P (1981)Google Scholar
  6. Storey P.J., MNRAS 195 27P (1981)Google Scholar
  7. Tondello G., Ap.J. 172, 771 (1972)CrossRefGoogle Scholar
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Copyright information

© Springer-Verlag 1984

Authors and Affiliations

  • Stephen A. Drake
    • 1
  • Jeffrey L. Linsky
    • 1
  1. 1.Joint Institute for Laboratory AstrophysicsUniversity of Colorado and National Bureau of StandardsBoulder

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