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- W2008004589 abstract "We present a set of 23 Doppler images of the spotted RS CVn star HR 1099 (V711 Tauri; HD 22468) obtained from 1981 to 1992. HR 1099 shows a large, cool polar spot that has persisted for the 11 yr of this study and other low-latitude spots that come and go on relatively short (less than 1 yr) timescales and can emerge anywhere on the star. The polar spot has variable protuberances that look very similar to the time-variable vertical extensions of the Sun's polar coronal hole. The area of the polar spot and its extensions shows marginal evidence of being variable, with a period of about 3 yr and an amplitude of about 1% that is perhaps indicative of a weak cycle, but this is not yet conclusive." @default.
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- W2008004589 date "1999-04-01" @default.
- W2008004589 modified "2023-09-24" @default.
- W2008004589 title "Doppler Imagery of the Spotted RS Canum Venaticorum Star HR 1099 (V711 Tauri) from 1981 to 1992" @default.
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- W2008004589 doi "https://doi.org/10.1086/313195" @default.
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