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A spot model for VW Cephei

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Abstract

An attempt is made to interpret the variations of the light curve of VW Cephei in terms of a spot model. A light curve which is (hopefully) free from starspot effects is constructed from Kwee's (1966a) observations, and is analysed by the light-curve synthesis method. Then, Kwee's individual light curves are further analysed by assuming that starspots exist on the surface of the primary component. Properties of starspots are briefly discussed.

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Authors and Affiliations

  1. Department of Earth Science and Astronomy, University of Tokyo, Japan

    A. Yamasaki

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  1. A. Yamasaki
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Yamasaki, A. A spot model for VW Cephei. Astrophys Space Sci 85, 43–58 (1982). https://doi.org/10.1007/BF00653431

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  • DOI: https://doi.org/10.1007/BF00653431

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