BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit
Thomas A. Baycroft, Alexandre Santerne, Amaury H.M.J. Triaud, Neda Heidari, Daniel Sebastian, Yasmin T. Davis, Alexandre C.M. Correia, Lalitha Sairam, Alix V. Freckelton, Aleyna Adamson, Isabelle Boisse, Gavin A.L. Coleman, Georgina Dransfield, Jo\~ao Faria, Salom\'e Grouffal

TL;DR
This paper reports the discovery of a new circumbinary giant planet, BEBOP-3b, using radial velocity data, and provides insights into its orbit, potential additional planets, and the binary star system's properties.
Contribution
First radial velocity detection of a previously unknown circumbinary planet, BEBOP-3b, with detailed analysis of its orbit and system stability.
Findings
BEBOP-3b has a mass of 0.56 M_Jup and orbits in 550 days with eccentricity 0.25.
Potential additional outer planet candidate with ~1400-day period.
Stable orbital solutions exist near the instability region for additional planets.
Abstract
Planetary systems orbiting close binaries are valuable testing grounds for planet formation and migration models. More detections with good mass measurements are needed. We present a new planet discovered during the BEBOP survey for circumbinary exoplanets using radial velocities. We use data taken with the SOPHIE spectrograph at the Observatoire de Haute-Provence, and perform a spectroscopic analysis to obtain high precision radial velocities. This planet is the first radial velocity detection of a previously unknown circumbinary system. The planet has a mass of and orbits its host binary in 550 days with an eccentricity of 0.25. Compared to most of the previously known circumbinary planets, BEBOP-3b has a long period (relative to the binary) and a high eccentricity. There also is a candidate outer planet with a day orbital period. We test the stability of…
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