Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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).
Язык оригинала | английский |
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Страницы (с-по) | 230-231 |
Число страниц | 2 |
Журнал | Proceedings of the International Astronomical Union |
DOI | |
Состояние | Электронная публикация перед печатью - 1 янв 2020 |
ID: 53086675