A lucky imaging multiplicity study of exoplanet host stars II

TL;DR

This study uses high-resolution imaging to identify and analyze stellar companions to exoplanet host stars, revealing new companions and providing data to understand how stellar multiplicity affects planet formation.

Contribution

It presents new high-resolution imaging observations that discover previously unknown stellar companions and offers detailed data on stellar multiplicity around exoplanet hosts.

Findings

Discovered 4 new stellar companions to exoplanet hosts.

Detected 11 new low-mass stellar companion candidates.

Provided new astrometric and photometric data for known binary systems.

Abstract

The vast majority of extrasolar planets are detected by indirect detection methods such as transit monitoring and radial velocity measurements. While these methods are very successful in detecting short-periodic planets, they are mostly blind to wide sub-stellar or even stellar companions on long orbits. In our study we present high resolution imaging observations of 63 exoplanet hosts carried out with the lucky imaging instrument AstraLux at the Calar Alto 2.2m telescope as well as with the new SPHERE high resolution adaptive optics imager at the ESO/VLT in the case of a known companion of specific interest. Our goal is to study the influence of stellar multiplicity on the planet formation process. We detected and confirmed 4 previously unknown stellar companions to the exoplanet hosts HD197037, HD217786, Kepler-21 and Kepler-68. In addition, we detected 11 new low-mass stellar companion candidates which must still be confirmed as bound companions. We also provide new astrometric and photometric data points for the recently discovered very close binary systems WASP-76 and HD2638. Furthermore, we show for the first time that the previously detected stellar companion to the HD185269 system is a very low mass binary. Finally we provide precise constraints on additional companions for all observed stars in our sample.