Time series analysis of V 368 Cephei photometry ?
نویسنده
چکیده
Our time series analysis of V 368 Cep photometry ascertains the rotation period of 2.d74 uniquely. The manifestations of starspot induced luminosity variations in this chromospherically active star include rapid light curve changes and differential rotation of about 3%. We conclude that the single rapidly rotating variable V 368 Cep is a high inclination K1v post T Tauri star.
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تاریخ انتشار 1999