Time series analysis of V 368 Cephei photometry

Details Time series analysis of V 368 Cephei photometry Time series analysis of V 368 Cephei photometry

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...350..513k&link_type=abstract

Astronomy and Astrophysics, v.350, p.513-516 (1999)

Astronomy and Astrophysics

Astrophysics

5

Stars: Variables: General, Stars: Individual: V 368 Cep, Techniques: Photometric

Scientific paper

Our time series analysis of {{V 368 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 {{V 368 Cep}} is a high inclination K1{v} post T Tauri star. Table~5 is only available in electronic form at CDS via anonymous ftp to edarc.u-strasbg.fr (130.79.1285) or via http://cdsweb.u-strasbg.fr/Abstract.html

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