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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
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.
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- III. Spectroscopy
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- Copyright © Reidel 1982