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- W3010131392 abstract "Some quadruple star systems in the hierarchical 2+2 configuration exhibit orbit-orbit resonances between the two compact binaries. We show that the most important resonances occur at period ratios of 1:1, 3:2 and 2:1. We describe the conditions required for capture and show that they can be satisfied at the 3:2 and 2:1 resonances in binaries that migrate significantly in semimajor axis after circularization, probably through magnetic braking or gravitational radiation." @default.
- W3010131392 created "2020-03-13" @default.
- W3010131392 creator A5083154228 @default.
- W3010131392 date "2020-03-09" @default.
- W3010131392 modified "2023-09-24" @default.
- W3010131392 title "Resonant capture in quadruple stellar systems" @default.
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- W3010131392 doi "https://doi.org/10.1093/mnras/staa643" @default.
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