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Blanketing Hypothesis and Light Variations of HD 27309
Published online by Cambridge University Press: 12 April 2016
Abstract
The influence of variable blanketing on the photometric variations of hot, silicon Ap star HD 27309 has been estimated. Spectrum variations in the visible are not the principal reason for the observed light variability, but flux redistribution from UV into visible fit well the observational data. An reference is made on the fulfillment of the variable blanketing assumptions at least for silicon Ap stars.
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- Section III - Magnetic CP Stars
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- Copyright © Reidel 1986