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On the Radiation Deficiency of Shell Stars in the Balmer Continuum

Published online by Cambridge University Press:  14 August 2015

J. N. Chkhikvadze
J. N. Chkhikvadze*
Affiliation:
Abastumani Astrophysical Observatory of the Academy of Sciences of Georgian SSR

Extract

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The present report gives the results of a statistical comparison of shell stars with normal Be stars to establish the differences in the parameters of the gaseous envelopes, such as the radiation power in the Paschen continuum and the optical depth of the envelopes in the Balmer continuum.

Type
III. Spectroscopy
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 141 - 146
Copyright
Copyright © Reidel 1982 

References

Mitropol'skij, A.A., Tekhnika Statisticheskikh Bychichlenij 1961, Moskva, Fizmatgyz.Google Scholar
Chkhkbadze, Ya. N., Astrofizika 1980, 16, no. 4.Google Scholar