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Recent Changes of the Be Star HD 58050
Published online by Cambridge University Press: 14 August 2015
Abstract
Emission line variations in 1961–1981 of the B2 star HD58050 are reported. Brightness variations are recalled. An estimation of the veiling effect given by continous emission of the envelope, observed in November 1980 in the Balmer lines, is given.
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- III. Spectroscopy
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- Copyright © Reidel 1982
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