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KIC 10486425: A Kepler eclipsing binary system with a pulsating component

Published online by Cambridge University Press:  18 February 2014

Filiz Kahraman Aliçavuş
Affiliation:
Department of Physics, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University TR-17020 Çanakkale, Turkey Astrophysics Research Centre and Observatory, Çanakkale Onsekiz Mart University, TR-17020 Çanakkale, Turkey email: filizkahraman01@gmail.com
Esin Soydugan
Affiliation:
Department of Physics, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University TR-17020 Çanakkale, Turkey Astrophysics Research Centre and Observatory, Çanakkale Onsekiz Mart University, TR-17020 Çanakkale, Turkey email: filizkahraman01@gmail.com
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Abstract

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We present frequency analysis of the Kepler light curve of KIC 10486425, an eclipsing binary system with a pulsating component. The parameters of the binary were obtained by modelling the light curve with the Wilson-Devinney program. The residuals from this modelling were subject to Fourier analysis which allowed us to detect 120 periodic terms characteristic for γ Dor-type pulsations. The dominant frequency of these changes amounts to 1.3189 d−1.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

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