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• W3100654928 startingPage "L19" @default.
• W3100654928 abstract "Some short-period, detached binary systems have recently been reported as experiencing very rapid orbital decay, much faster than is expected from the angular-momentum loss caused by gravitational radiation alone. As these systems contain fully convective stars, magnetic braking is not believed to be operative, making the large orbital-period derivative puzzling. Here, we explore whether a resonant interaction between the binary and a surrounding circumbinary (CB) disk could account for the observed orbital decay. Our calculations indicate that the observed orbital-period derivatives in seven detached binaries can be produced by the resonant interaction between the binary and a CB disk if the latter has a mass in the range of , which is of the same order as the inferred disk mass () in the post-common-envelope binary NN Ser." @default.
• W3100654928 created "2020-11-23" @default.
• W3100654928 creator A5016854610 @default.
• W3100654928 creator A5035012048 @default.
• W3100654928 date "2017-03-07" @default.
• W3100654928 modified "2023-10-18" @default.
• W3100654928 title "Rapid Orbital Decay in Detached Binaries: Evidence for Circumbinary Disks" @default.
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• W3100654928 doi "https://doi.org/10.3847/2041-8213/aa624a" @default.
• W3100654928 hasPublicationYear "2017" @default.
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