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Emission Features of Several Be Stars as Related to Their Luminosity Class and Spectral Type

Published online by Cambridge University Press:  14 August 2015

H. Hubert  and
M. Th. Chambon
H. Hubert
Affiliation:
Observatoire de Meudon, France
M. Th. Chambon
Affiliation:
Observatoire de Meudon, France

Extract

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At the Haute Provence Observatory, a survey of the Be stars brighter than the seventh magnitude was initiated by Herman and her collaborators twenty years ago.

Type
Part 1: Observations of Be Stars
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 33 - 36
Copyright
Copyright © Reidel 1976 

References

Delplace, A. M. and Hubert, H.: 1973, Compt. Rend. Acad. Sci. Paris 277, 575.Google Scholar
Delplace, A. M. and Hubert, H.: 1975, Astron. Astrophys. 38, 75.Google Scholar
Herman, R.: 1973, in Fehrenbach, Ch. and Westerlund, B. E. (eds.): ‘Spectral Classification and Multicolour Photometry’, IAU Symp. 50, p. 17.Google Scholar
Herman, R.: 1974, private communication.Google Scholar
Hubert, H.: 1971, Astron. Astrophys. 11, 100.Google Scholar
Hubert, H.: 1973, Astron. Astrophys. Suppl. 9, 133.Google Scholar
Rountree-Lesh, J.: 1968, Astrophys. J. Suppl. 16, 371.CrossRefGoogle Scholar