V368 Cep UBVRI time series

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33500513
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/350/513
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/350/513
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/350/513
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/350/513
Provenance
Creator Kahanpaa J.; Jetsu L.; Alha L.; Ezhkova O.V.; Grankin K.N.; Hackman T.,Ibragimov M.A.; Kokko M.; Kondratiev V.B.; Laakso T.; Lindroos O.,Mel'nikov S.Yu.; Nikula P.O.; Schultz J.; Shevchenko V.S.; Torppa J.,Tuominen I.; Tyynela J.; Virtanen J.
Publisher CDS
Publication Year 1999
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy