HD183648: a Kepler eclipsing binary with anomalous ellipsoidal variations and a pulsating component
1 ELTE Gothard Astrophysical Observatory, H-9704 Szombathely, Szent Imre herceg út 112, Hungary
2 Konkoly Observatory, MTA CSFK, H-1121 Budapest, Konkoly Thege M. út 15-17, Hungary
3 Baja Astronomical Observatory, H-6500 Baja, Szegedi út, Kt. 766, Hungary
4 Department of Astronomy, Center for Space Research, Cornell University, Ithaca, NY 14853, USA
5 Department of Physics, University of Zagreb, Bijenička cesta 32, 10000 Zagreb, Croatia
6 Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK
7 Department of Astrophysics and Planetary Science, Villanova University, 800 Lancaster Ave, Villanova PA 19085, USA
8 Apache Point Observatory, Sunspot NM 88349, USA
9 Astrophysics Group, Keele University, Newcastle-under-Lyme, ST5 5BG, UK
10 Astronomical Department of Eötvös University, H-1118 Pázmány Pèter sètány. 1/A, Budapest, Hungary
a e-mail: email@example.com
Published online: 23 September 2015
KIC 8560861 (HD 183648) is a marginally eccentric (e = 0.05) eclipsing binary with an orbital period of Porb = 31.973 d, exhibiting mmag amplitude pulsations on time scales of a few days. We present the results of the complex analysis of high and medium-resolution spectroscopic data and Kepler Q0 – Q16 long cadence photometry.
© Owned by the authors, published by EDP Sciences, 2015
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