FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION

FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION

Stellar companions can influence the formation and evolution of planetary systems, but there are currently few observational constraints on the properties of planet-hosting binary star systems. We search for stellar companions around 77 transiting hot Jupiter systems to explore the statistical prope...

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Bibliographic Details
Main Authors: Ngo, Henry, Knutson, Heather A., Hinkley, Sasha, Bryan, Marta, Crepp, Justin R., Batygin, Konstantin, Crossfield, Ian, Hansen, Brad, Howard, Andrew W., Johnson, John A., Mawet, Dimitri, Morton, Timothy D., Muirhead, Philip S., Wang, Ji
Other Authors: Univ Arizona, Lunar & Planetary Lab
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
binaries: close
binaries: eclipsing
methods: observational
planetary systems
planets and satellites: dynamical evolution and stability
techniques: high angular resolution
Online Access:http://hdl.handle.net/10150/621385
http://arizona.openrepository.com/arizona/handle/10150/621385

Internet

http://hdl.handle.net/10150/621385
http://arizona.openrepository.com/arizona/handle/10150/621385

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