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- W2790363872 abstract "We investigate the long-term dynamics of planetesimals in debris disks in models with the parameters of the binary star systems Kepler-16, Kepler-34, and Kepler-35 with planets. Our calculations show that the formation of a stable ring coorbital with the planet is possible for Kepler-16 and Kepler-35. In Kepler-34 significant orbital eccentricities of the binary system and the planet can prevent the formation of such a structure. The detection of circumbinary ring-like structures in observations of binary star systems can be evidence for the existence of planets retaining coorbital rings of dust and planetesimals." @default.
- W2790363872 created "2018-03-29" @default.
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- W2790363872 date "2018-02-01" @default.
- W2790363872 modified "2023-10-18" @default.
- W2790363872 title "Simulations of the Dynamics of the Debris Disks in the Systems Kepler-16, Kepler-34, and Kepler-35" @default.
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- W2790363872 doi "https://doi.org/10.1134/s1063773718010012" @default.
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