Limits on stellar companions to exoplanet host stars with eccentric planets

Kane, Stephen R. and Howell, Steve B. and Horch, Elliott P. and Feng, Ying and Hinkel, Natalie R. and Ciardi, David R. and Everett, Mark E. and Howard, Andrew W. and Wright, Jason T. (2014) Limits on stellar companions to exoplanet host stars with eccentric planets. The Astrophysical Journal, 785 (2). pp. 93-102. ISSN 0004-637X

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Abstract

Though there are now many hundreds of confirmed exoplanets known, the binarity of exoplanet host stars is not well understood. This is particularly true of host stars that harbor a giant planet in a highly eccentric orbit since these are more likely to have had a dramatic dynamical history that transferred angular momentum to the planet. Here we present observations of four exoplanet host stars that utilize the excellent resolving power of the Differential Speckle Survey Instrument on the Gemini North telescope. Two of the stars are giants and two are dwarfs. Each star is host to a giant planet with an orbital eccentricity >0.5 and whose radial velocity (RV) data contain a trend in the residuals to the Keplerian orbit fit. These observations rule out stellar companions 4-8 mag fainter than the host star at passbands of 692 nm and 880 nm. The resolution and field of view of the instrument result in exclusion radii of 0.″05-1.″4, which excludes stellar companions within several AU of the host star in most cases. We further provide new RVs for the HD 4203 system that confirm that the linear trend previously observed in the residuals is due to an additional planet. These results place dynamical constraints on the source of the planet's eccentricities, place constraints on additional planetary companions, and inform the known distribution of multiplicity amongst exoplanet host stars.


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Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Additional Information: Access to published version in accordance with the copyright policy of the publisher.
Faculty / Department / School: No Faculty
Date Deposited: 02 Jun 2017 07:08
Last Modified: 27 Jun 2017 00:55
Uncontrolled Keywords: planetary systems; stars: individual (HD 4203, HD 168443, HD 1690, HD 137759); techniques: high angular resolution; techniques: Radial velocities;
Fields of Research : 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Socio-Economic Objective: E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Identification Number or DOI: 10.1088/0004-637X/785/2/93
URI: http://eprints.usq.edu.au/id/eprint/32116

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