A new eclipsing binary system with a pulsating component detected by CoRoT
K. Sokolovsky, C. Maceroni, M. Hareter, C. Damiani, L. Balaguer-Nunez,, and I. Ribas

TL;DR
This paper reports the discovery of a new eclipsing binary system with a pulsating component observed by CoRoT, revealing detailed orbital and pulsation characteristics and suggesting a gamma Doradus classification.
Contribution
It presents the first detailed analysis of CoRoT 102980178, identifying its binary and pulsation properties and proposing its classification as a gamma Doradus type pulsator.
Findings
Discovered a semi-detached eclipsing binary with pulsations.
Identified primary star as the pulsating component.
Detected pulsation frequencies at 2.75 c/d and 0.21 c/d.
Abstract
We report the discovery of CoRoT 102980178 (R.A.= 06:50:12.10, Dec.= -02:41:21.8, J2000) an Algol-type eclipsing binary system with a pulsating component (oEA). It was identified using a publicly available 55 day long monochromatic lightcurve from the CoRoT initial run dataset (exoplanet field). Eleven consecutive 1.26m deep total primary and the equal number of 0.25m deep secondary eclipses (at phase 0.50) were observed. The following light elements for the primary eclipse were derived: HJD_MinI= 2454139.0680 + 5.0548d x E. The lightcurve modeling leads to a semidetached configuration with the photometric mass ratio q=0.2 and orbital inclination i=85 deg. The out-of-eclipse lightcurve shows ellipsoidal variability and positive O'Connell effect as well as clear 0.01m pulsations with the dominating frequency of 2.75 c/d. The pulsations disappear during the primary eclipses, which…
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