VizieR Online Data Catalog: V368 Cep UBVRI time series (Kahanpaa+, 1999)
Abstract
Our time series analysis of V368 Cep photometry ascertains the rotation period of 2.74d 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 V368 Cep is a high inclination K1V post T Tauri star. (1 data file).
- Publication:
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VizieR Online Data Catalog
- Pub Date:
- September 1999
- DOI:
- 10.26093/cds/vizier.33500513
- Bibcode:
- 1999yCat..33500513K
- Keywords:
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- Stars: variable;
- Photometry: UBVRI