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Light curve solution and orbital period analysis of the contact binary V842 Herculis
Author(s) -
Selam S. O.,
Albayrak B.,
Şenavci H. V.,
Aksu O.
Publication year - 2005
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.200510400
Subject(s) - light curve , physics , astrophysics , orbital period , contact binary , diagram , mass ratio , orbital inclination , photoelectric effect , binary number , binary star , stars , optics , statistics , mathematics , arithmetic
New photoelectric BV light curves were obtained for the neglected eclipsing binary V842 Her at the TÜBİTAK 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 d P /d t = 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 0.4 M ⊙ 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. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)