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Binarity of Pleione and its influence on the circumstellar disk
Published online by Cambridge University Press: 30 December 2019
Abstract
Pleione is a classical Be star well known for its cyclic transitions between Be-, shell- and normal B spectral phases. Its nature as a binary system was discussed by McAlister et al. (1989), Gies et al. (1990), Luthardt & Menchenkova (1994) and Nemravova et al (2010). We present the results that trace the evolution of the dimensions of the circumstellar disk of Pleione that are related to the binary system.
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- © International Astronomical Union 2019