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UBVRI polarimetry of WR stars
Published online by Cambridge University Press: 07 August 2017
Abstract
Five-colour polarimetry of a sample of twelve southern WR stars is presented. We suggest a method for separation the interstellar and intrinsic polarization components. Based on the observed data, a dependence of λmax on the terminal velocity v∞ is suggested. Its possible origin could be related to circumstellar envelopes.
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- Session IV - poster summaries
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- Copyright © Kluwer 1995