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Statistical Properties of Be Stars

Published online by Cambridge University Press:  14 August 2015

A.M. Hubert-Delplace
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France
M. Jaschek
Affiliation:
Observatoire de Strasbourg, 11, rue de l'Université, 67000 Strasbourg, France
H. Hubert
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France
M. Th. Chambon
Affiliation:
DEPEG, Observatoire de Paris, 92190 Meudon, France

Abstract

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The emission features of 140 Be stars described in “An Atlas of Be stars” are briefly reviewed. The time scale of the emission variations are determined for about 35 stars. For several stars we estimated, on the Hβ line, the V/R ratio of the two emission components.

Type
III. Spectroscopy
Copyright
Copyright © Reidel 1982 

References

Alvarez, M., Schuster, W.: 1981, to be published in Revista Mexicana de Astronomia y Astrophysica.Google Scholar
Ferrari-Toniolo, M., Natali, G., Persi, P., Spada, G.: 1977, Astron. Astrophys. 61, 47.Google Scholar
Golay, M.: 1979, Publ. de l'Obs. Astr. de Strasbourg, 6, 101.Google Scholar
Harmanec, P., Horn, J., Koubsky, P., Zdársky, F., Kriz, S., Pavlovski, K.: 1980, Bull. Astron. Inst. Czech. 31, 144.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
Sharov, A.S., Lyuty, V.M.: 1975 IAU Symposium N°70, p. 105.Google Scholar
Yilmaz, N.,;1968, thèse d'Université, Paris, unpublished Google Scholar