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- W321656938 abstract "Context. Hot subdwarf-B stars in long-period binaries are found to be on eccentric orbits, even though current binary-evolution theory predicts these objects to be circularised before the onset of Roche-lobe overflow (RLOF)." @default.
- W321656938 created "2016-06-24" @default.
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- W321656938 date "2015-06-26" @default.
- W321656938 modified "2023-10-12" @default.
- W321656938 title "Testing eccentricity pumping mechanisms to model eccentric long-period sdB binaries with MESA" @default.
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- W321656938 doi "https://doi.org/10.1051/0004-6361/201526019" @default.
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