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Resonant multi-lane patterns in circumbinary young debris disks

Published online by Cambridge University Press:  13 January 2020

Tatiana V. Demidova  and
Ivan I. Shevchenko Open the ORCID record for Ivan I. Shevchenko [Opens in a new window]
Tatiana V. Demidova
Affiliation:
Pulkovo Observatory, Russian Academy of Sciences, 196140 Saint Petersburg, Russia email: proxima1@list.ru
Ivan I. Shevchenko
Affiliation:
Pulkovo Observatory, Russian Academy of Sciences, 196140 Saint Petersburg, Russia email: proxima1@list.ru
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Abstract

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Formation of resonant multi-lane patterns in circumbinary young debris disks with planets is considered in a set of representative massively simulated models. We find that the long term-stable resonant patterns are generically formed, shepherded by embedded planets. The patterns are multi-lane, i.e., they consist of several concentric rings. Statistical dependences of their parameters on the planetary parameters are recovered. Relevant additional massive simulations of planetesimal disks in systems with parameters of Kepler-16, 34, and 35 are accomplished and described. We find that co-orbital patterns generically form in systems with moderate orbital eccentricities of the binary’s and planetary orbits (like in Kepler-16 and 35 cases).

Keywords

Methods: n-body simulationsplanetary systems: protoplanetary disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S345: Origins: From the Protosun to the First Steps of Life , August 2018 , pp. 230 - 231
Copyright
© International Astronomical Union 2020 

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