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Recent Changes of the Be Star HD 58050

Published online by Cambridge University Press:  14 August 2015

A.M. Hubert-Delplace
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France
H. Hubert
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France
D. Ballereau
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France
M. Th. Chambon
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France

Abstract

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Emission line variations in 1961–1981 of the B2 star HD58050 are reported. Brightness variations are recalled. An estimation of the veiling effect given by continous emission of the envelope, observed in November 1980 in the Balmer lines, is given.

Type
III. Spectroscopy
Copyright
Copyright © Reidel 1982 

References

Burbidge, E.M., Burbidge, G.R.: 1953, Astrophys. J. 118, 262.Google Scholar
Hubert-Delplace, A.M., Hubert, H.: 1979, An Atlas of Be stars.Google Scholar
Jaschek, M., Hubert-Delplace, A.M., Hubert, H., Jaschek, C.: 1980, Astron. Astrophys. Suppl. Ser., 42, 103.Google Scholar
Kogure, T.: 1970, Astron. Astrophys. 1, 253.Google Scholar
Tcheng-Mao-Lin, : 1946, Ann. Astron. 9, 120.Google Scholar
Uesugi, A.: 1978, Revised Catalogue of Stellar rotational velocities-Preliminary Edition.Google Scholar