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Stellar Pulsation pp 96–101Cite as

Empirical-theoretical modeling of Be variable mass-loss via variable: Photospheric mass-outflow; Coronal opacity; Radiation-amplified wind-piston, driving pulsating cool-envelope

  • B Star Pulsations
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Part of the book series: Lecture Notes in Physics ((LNP,volume 274))

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References

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Author information

Authors and Affiliations

  1. Obs.Paris, Paris

    Vera Doazan

  2. Radiophysics,Inc, Paris

    Richard N. Thomas

Authors
  1. Vera Doazan
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  2. Richard N. Thomas
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Editor information

A. N. Cox W. M. Sparks S. G. Starrfield

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© 1987 Springer-Verlag

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Doazan, V., Thomas, R.N. (1987). Empirical-theoretical modeling of Be variable mass-loss via variable: Photospheric mass-outflow; Coronal opacity; Radiation-amplified wind-piston, driving pulsating cool-envelope. In: Cox, A.N., Sparks, W.M., Starrfield, S.G. (eds) Stellar Pulsation. Lecture Notes in Physics, vol 274. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-17668-3_182

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  • DOI: https://doi.org/10.1007/3-540-17668-3_182

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-17668-8

  • Online ISBN: 978-3-540-47754-9

  • eBook Packages: Springer Book Archive

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