The transiting circumbinary planets Kepler-34 b and Kepler-35 b

Most Sun-like stars in the Galaxy reside in gravitationally bound pairs of stars (binaries). Although long anticipated the existence of a ‘circumbinary planet’ orbiting such a pair of normal stars was not definitively established until the discovery9 of the planet transiting (that is, passing in fro...

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Bibliographic Details
Main Author: Winn, Joshua Nathan
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Nature Publishing Group 2013
Online Access:http://hdl.handle.net/1721.1/77037
https://orcid.org/0000-0002-4265-047X