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Variations of the C III 5696 Å Emission Line in Wolf-Rayet Stars

Published online by Cambridge University Press:  14 August 2015

J. D. Schumann  and
W. Seggewiss
J. D. Schumann
Affiliation:
Observatorium Hoher List der Universitäts-Sternwarte, Bonn, F.R.G.
W. Seggewiss
Affiliation:
Observatorium Hoher List der Universitäts-Sternwarte, Bonn, F.R.G.

Abstract

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Slow and rapid fluctuations of emission and absorption features of the C III emission line at λ 5696 Å in WC stars are described. They might be attributed to moving clouds in the expanding stellar envelope.

Type
Part 5 / Wolf-Rayet Stars
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 299 - 302
Copyright
Copyright © Reidel 1975 

References

Gauzit, J.: 1966, Compt. Rend. Acad. Sci. Paris B262, 1309.Google Scholar
Nussbaumer, H.: 1971, Astrophys. J. 170, 93.CrossRefGoogle Scholar
Schumann, J. D.: 1971, Messtechnik 79, 174 and 189.Google Scholar
Seggewiss, W.: 1974, Astron. Astrophys. 31, 211.Google Scholar
Smith, L. F.: 1968, Monthly Notices Roy. Astron. Soc. 138, 109.CrossRefGoogle Scholar
Struve, O.: 1944, Astrophys. J. 100, 384.CrossRefGoogle Scholar
Underhill, A. B.: 1957, Astrophys. J. 126, 28.CrossRefGoogle Scholar