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...
Main Authors: | , , , , , |
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Language: | en |
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OXFORD UNIV PRESS
2018
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Online Access: | http://hdl.handle.net/10150/627133 http://arizona.openrepository.com/arizona/handle/10150/627133 |