Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries

The orbital parameters of binaries at intermediate periods (10(2)-10(3) d) are difficult to measure with conventional methods and are very incomplete. We have undertaken a new survey, applying our pulsation timing method to Kepler light curves of 2224 main-sequence A/F stars and found 341 non-eclips...

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Bibliographic Details
Main Authors: Murphy, Simon J, Moe, Maxwell, Kurtz, Donald W, Bedding, Timothy R, Shibahashi, Hiromoto, Boffin, Henri M J
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: OXFORD UNIV PRESS 2018
Subjects:
Online Access:http://hdl.handle.net/10150/627133
http://arizona.openrepository.com/arizona/handle/10150/627133