V368 Cep UBVRI time series Virtual Observatory Resource

Authors

1. Kahanpaa J.
2. Jetsu L.
3. Alha L.
4. Ezhkova O.V.
5. Grankin K.N.
6. Hackman T.,Ibragimov M.A.
7. Kokko M.
8. Kondratiev V.B.
9. Laakso T.
10. Lindroos O.,Mel'nikov S.Yu.
11. Nikula P.O.
12. Schultz J.
13. Shevchenko V.S.
14. Torppa J.,Tuominen I.
15. Tyynela J.
16. Virtanen J.

Published by

CDS

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.

Keywords

1. variable-stars
2. infrared-photometry
3. visible-astronomy
4. Wide-band photometry

Bibliographic source Bibcode

1999A&A...350..513K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/350/513

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/350/513

Document Object Identifer DOI

doi:10.26093/cds/vizier.33500513

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/350/513
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/350/513
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/350/513

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).