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Observational Evidence for Large-Scale Spot Activity on the Primary Component of XY Ursae Majoris
Published online by Cambridge University Press: 14 August 2015
Abstract
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Extensive pe- and spectroscopic observations of the short period eclipsing binary XY UMa within the last four years confirm the star spot and stellar activity model, which was presented in 1975.
- Type
- VII. The RS Canum Venaticorum Stars
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- Copyright © Reidel 1980
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