Influence of spots on O-C diagrams of close eclipsing binary stars

Details Influence of spots on O-C diagrams of close eclipsing binary stars Influence of spots on O-C diagrams of close eclipsing binary stars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..292..163r&link_type=abstract

Interplay of Periodic, Cyclic and Stochastic Variability in Selected Areas of the H-R Diagram. Edited by C. Sterken, ASP Conf. S

Astronomy and Astrophysics

Astronomy

Scientific paper

The influence of dark spots in close eclipsing binaries is examined.
We show that the O'Connell efect is much greater if the spot lies on
the primary component. It is also shown that this phase shift is not
capable of modulating variations in the O-C diagrams of close eclipsing
binaries. This means that spots cannot cause orbital period changes.

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