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The FeII λ5317 line profile of nine Be stars(*)

Published online by Cambridge University Press:  26 May 2016

D. Ballereau
Affiliation:
Observatoire de Paris-Meudon - 92195 Meudon Cedex, France
J. Chauville
Affiliation:
Observatoire de Paris-Meudon - 92195 Meudon Cedex, France
J. Zorec
Affiliation:
Institut d'Astrophysique - 98bis, Bd. Arago, 75014 Paris, France

Abstract

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Our aim is to analyze the FeII λ5317 emission line of nine Be stars recorded in 1990, to deduce some constraints on the modeling of their envelope and to compare them to the results obtained in 1985 and 1987 by other authors.

Type
5. Be Stars: Spectroscopy and Photometry
Copyright
Copyright © Kluwer 1994 

References

Dachs, J., Hummel, W., Hanuschik, R.W.: 1992, Astron. Astrophys. Suppl. 95, 437 Google Scholar
Hanuschik, R.W.: 1987, Astron. Astrophys. 173, 299 Google Scholar
Huang, S.-S.: 1972, Astrophys. J. 171, 549 Google Scholar
Hubert, A.-M., Hubert, H., Floquet, M. et al.: 1989, in Delache, P., Laloe, S., Magnan, C. and Tran Thanh Van, J., ed(s)., Modeling the Stellar Environment: How and Why? , Editions Frontières, 263 Google Scholar
Slettebak, A., Collins, G.W. II, Truax, R.: 1992, Astrophys. J. Suppl. 81, 335 Google Scholar