Light curve solution and orbital period analysis of the contact binary V842 Herculis

Details Light curve solution and orbital period analysis of the contact binary V842 Herculis Light curve solution and orbital period analysis of the contact binary V842 Herculis

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005an....326..746s&link_type=abstract

Astronomische Nachrichten, Vol.326, Issue 8, p.746-753

Astronomy and Astrophysics

Astronomy

2

Binaries: Close, Binaries: Eclipsing, Stars: Individual (V842 Her), Stars: Fundamental Parameters

Scientific paper

New photoelectric BV light curves were obtained for the neglected eclipsing binary V842 Her at the TÜB{İTAK National Observatory (TUG) and studied for the first time in detail to determine the orbital parameters and geometry of the system. The solutions obtained simultaneously for the new light curves and the radial velocity curves in the literature by using the Wilson-Devinney code reveal a typical W-type contact system. The light curves exhibit the so-called O'Connell effect which the level of the primary maxima being higher than that of the secondary ones in both pass-bands. The O'Connell effect in the light curves is explained in terms of a dark-spot located on the more massive component which makes the more massive larger component slightly cooler than the less massive smaller one. The O-C diagram constructed for all available times of minima of V842 Her exhibits a cyclic character superimposed on a quadratic variation. The quadratic character yields a orbital period increase with a rate of dP/dt=7.76×10-7 days yr-1 which can be attributed to the mass exchange/loss mechanism in the system. By assuming the presence of a gravitationally bound third body in the system, the analysis of the cyclic nature in the O-C diagram revealed a third body with mass of 0.4M\sun orbiting around the eclipsing pair. The possibility of magnetic activity cycle effect as a cause for the observed cyclic variation in the O-C diagram was also discussed.

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