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Le Spectre des Etoiles Oe dans le Rouge et le Proche Infrarouge
Published online by Cambridge University Press: 14 August 2015
Abstract
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Among the 0 stars, Conti and Leep (1974) define the Oe class as those stars showing emission in the hydrogen lines but without emission in N III or 4686 He II.
In the blue-red region, aside from the presence of Lambda 4542 in absorption, the overall appearance is similar to Be stars. So far no Oe star has been observed until 1.1 μ: the aim of this paper is to fill this gap. We present observations of Oe stars in the near infra-red region as well as new observations of Hα profiles.
- Type
- IV. Infrared Observations
- Information
- Copyright
- Copyright © Reidel 1982
References
Frost, S.A. and Conti, P.S.: 1976,in Slettebak, A.(ed.), Be and shell stars, D. Reidel Publ. Co., Dordrecht-Holland, 139.CrossRefGoogle Scholar
Polidan, R.S. and Peters, G.J.: 1976,in Slettebak, A.(ed.), Be and shell stars, D. Reidel Publ. Co., Dordrecht-Holland, 59.Google Scholar
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