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Simulations of the Dynamics of the Debris Disks in the Systems Kepler-16, Kepler-34, and Kepler-35

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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.

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Authors and Affiliations

  1. Pulkovo Astronomical Observatory, Russian Academy of Sciences, Pulkovskoe sh. 65, St. Petersburg, 196140, Russia

    T. V. Demidova & I. I. Shevchenko

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  1. T. V. Demidova
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  2. I. I. Shevchenko
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Correspondence to T. V. Demidova.

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Original Russian Text © T.V. Demidova, I.I. Shevchenko, 2018, published in Pis’ma v Astronomicheskii Zhurnal, 2018, Vol. 44, No. 2, pp. 140–147.

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Demidova, T.V., Shevchenko, I.I. Simulations of the Dynamics of the Debris Disks in the Systems Kepler-16, Kepler-34, and Kepler-35. Astron. Lett. 44, 119–125 (2018). https://doi.org/10.1134/S1063773718010012

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