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The Variations of the Hα line of HD199178
Published online by Cambridge University Press: 12 April 2016
Abstract
Changes of emission cause variations of the Hα absorption line of HD 199178. The correlation with the simultaneous light curve may depend on the relative strength of the axisymmetric and non-axisymmetric components of the evolving spot configurations.
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- Part IV Stellar activity
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- Copyright © Springer-Verlag 1991