The Photometric Behaviour of Bh-Virginis

Details The Photometric Behaviour of Bh-Virginis The Photometric Behaviour of Bh-Virginis

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..245a&link_type=abstract

Astrophysics and Space Science, Volume 169, Issue 1-2, pp. 245-246

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Visible light curves of the RS CVn short-period system BH Vir, collected over 26 years, have been analyzed.B-V colours indicate that the primary minimum is normally redder than one would expect, assuming the spectroscopic classification of the system components, while the secondary yielded bluer. A qualitative comparison of the different light curves, suggests that not only cool starspots are the reason of the observed variability.

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