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Gross Structural Pattern for the Atmospheres of Be, and Some Closely Related, Stars

Published online by Cambridge University Press:  14 August 2015

V. Doazan ,
R. Stalio  and
R. N. Thomas
V. Doazan
Affiliation:
Observatoire de Paris, Osservatorio di Trieste, Institut d'Astrophysique, Paris
R. Stalio
Affiliation:
Observatoire de Paris, Osservatorio di Trieste, Institut d'Astrophysique, Paris
R. N. Thomas
Affiliation:
Observatoire de Paris, Osservatorio di Trieste, Institut d'Astrophysique, Paris

Extract

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Abstracted comparison of Struve's 1942 quasi-empirical model of the shell-atmosphere of Be and similar stars, based on visual data and quasi-radiative equilibrium, to that demanded by current visual+nonvisual data, requiring nonradiative+mass fluxes characterized by variability and individuality.

Type
VIII. Atmospheric Models
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 489 - 491
Copyright
Copyright © Reidel 1982 

References

Edlen, B., 1942, Zs. Ap. 22, 30 Google Scholar
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Redman, R.O., 1942, MNRAS, 102, 134, 140 CrossRefGoogle Scholar
Struve, O., 1942, Ap. J. 95, 134 CrossRefGoogle Scholar
NASA-CNRS monograph series, Nonthermal Structure of Stellar Atmospheres: 1981 et seq.Google Scholar
Hack, M., Stalio, R., Cataclysmic Stars, 1982.Google Scholar
Thomas, R.N., Stellar Atmospheres, 1982.Google Scholar
Underhill, A.B., Doazan, V., B and Be Stars, 1981.Google Scholar