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The Variable Shell Phase of HD 184279 between 1976 and 1980
Published online by Cambridge University Press: 14 August 2015
Abstract
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The variable shell (H, HeI, FeIII and once ionized other metals) B0.5 star HD 184279 presents variations of radial velocity and line profiles with a cycle of about 4 years. Some correlations between photometric and spectroscopic data are found. A comparison with 48 Lib and ζ Tau is given.
- Type
- III. Spectroscopy
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- Copyright
- Copyright © Reidel 1982
References
Alvarez, M. and Schuster, W.: 1981, to be published in
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Jaschek, M., Hubert-Delplace, A.M., Hubert, H., Jaschek, C., A Classification of Be Stars, Astron. and Astrophys., Suppl. Ser., 42, 103.Google Scholar
Uesugi, A.: 1978, Revised Catalogue of Stellar Rotational Velocities-Preliminary Edition.Google Scholar
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