The Photometric Behaviour of Bh-Virginis

Bibcode
1990Ap&SS.169..245A
DOI
10.1007/BF00640724
Arévalo, M. J.; Lázaro, C.
Referencia bibliográfica

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

Fecha de publicación:
7
1990
Revista
Astrophysics and Space Science
Número de autores
2
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
2
Descripción
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.
Tipo
Sin árbitro

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