The Light Curve Variations of The Active Binaries With Hot Subdwarf Component

Details The Light Curve Variations of The Active Binaries With Hot Subdwarf Component The Light Curve Variations of The Active Binaries With Hot Subdwarf Component

2006-07-10

arxiv.org/abs/astro-ph/0607183v1

Astronomy and Astrophysics

Astrophysics

Published in Proceedings of the 13th Young Scientists' Conference on Astronomy and Space Physics, held in Kyiv, Ukraine, April

Scientific paper

We present the light curve variations of the two active binaries with hot
subdwarf component. According to the brightness variations outside of the
eclipses, the giant components of the systems are chromospherically active
stars. The dark and cool active structures on this components cause the
variations of the total light of the systems.

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