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• W1938358624 endingPage "9269" @default.
• W1938358624 startingPage "9264" @default.
• W1938358624 abstract "The discovery of transiting circumbinary planets by the Kepler mission suggests that planets can form efficiently around binary stars. None of the stellar binaries currently known to host planets has a period shorter than 7 d, despite the large number of eclipsing binaries found in the Kepler target list with periods shorter than a few days. These compact binaries are believed to have evolved from wider orbits into their current configurations via the so-called Lidov-Kozai migration mechanism, in which gravitational perturbations from a distant tertiary companion induce large-amplitude eccentricity oscillations in the binary, followed by orbital decay and circularization due to tidal dissipation in the stars. Here we explore the orbital evolution of planets around binaries undergoing orbital decay by this mechanism. We show that planets may survive and become misaligned from their host binary, or may develop erratic behavior in eccentricity, resulting in their consumption by the stars or ejection from the system as the binary decays. Our results suggest that circumbinary planets around compact binaries could still exist, and we offer predictions as to what their orbital configurations should be like." @default.
• W1938358624 created "2016-06-24" @default.
• W1938358624 creator A5007773051 @default.
• W1938358624 creator A5088598643 @default.
• W1938358624 date "2015-07-09" @default.
• W1938358624 modified "2023-10-16" @default.
• W1938358624 title "Survival of planets around shrinking stellar binaries" @default.
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• W1938358624 doi "https://doi.org/10.1073/pnas.1505671112" @default.
• W1938358624 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/4522779" @default.
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• W1938358624 hasPublicationYear "2015" @default.
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