Abstract
V andB observations of V711 Tauri (HR 1099) for the year 1982–1983 are presented. The light curves made with the data of this season are compared with those of the previous observations of the 1981–1982 season. The single-peaked maximum light had shifted slightly and the peak amplitude had decreased to 0.04 mag. inV. No clear sign of colour,B−V, variation in comparison with the low temperature dark-spot is detected.
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Nha, IS., Oh, JY. Light curves of V711 Tauri (HR 1099). Astrophys Space Sci 118, 299–303 (1986). https://doi.org/10.1007/BF00651140
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DOI: https://doi.org/10.1007/BF00651140