Revising Properties of Planet–Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems

Revising Properties of Planet–Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems

Binary stars are ubiquitous; the majority of solar-type stars exist in binaries. Exoplanet occurrence rate is suppressed in binaries, but some multiples do still host planets. Binaries cause observational biases in planet parameters, with undetected multiplicity causing transiting planets to appear...

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Bibliographic Details
Main Authors: Kendall Sullivan, Adam L. Kraus, Daniel Huber, Erik A. Petigura, Elise Evans, Trent Dupuy, Jingwen Zhang, Travis A. Berger, Eric Gaidos, Andrew W. Mann
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Exoplanets
Extrasolar rocky planets
Binary stars
Online Access:https://doi.org/10.3847/1538-3881/acbdf9

Internet

https://doi.org/10.3847/1538-3881/acbdf9

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