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Resonant multi-lane patterns in circumbinary young debris disks. / Demidova, Tatiana V.; Shevchenko, Ivan I.

в: Proceedings of the International Astronomical Union, 01.01.2020, стр. 230-231.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Demidova, TV & Shevchenko, II 2020, 'Resonant multi-lane patterns in circumbinary young debris disks', Proceedings of the International Astronomical Union, стр. 230-231. https://doi.org/10.1017/S1743921318008220

APA

Demidova, T. V., & Shevchenko, I. I. (2020). Resonant multi-lane patterns in circumbinary young debris disks. Proceedings of the International Astronomical Union, 230-231. https://doi.org/10.1017/S1743921318008220

Vancouver

Demidova TV, Shevchenko II. Resonant multi-lane patterns in circumbinary young debris disks. Proceedings of the International Astronomical Union. 2020 Янв. 1;230-231. https://doi.org/10.1017/S1743921318008220

Author

Demidova, Tatiana V. ; Shevchenko, Ivan I. / Resonant multi-lane patterns in circumbinary young debris disks. в: Proceedings of the International Astronomical Union. 2020 ; стр. 230-231.

BibTeX

@article{26a87a5cea9b4b8e96024c63924350fb,
title = "Resonant multi-lane patterns in circumbinary young debris disks",
abstract = "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 simulations, planetary systems: Protoplanetary disks",
author = "Demidova, {Tatiana V.} and Shevchenko, {Ivan I.}",
year = "2020",
month = jan,
day = "1",
doi = "10.1017/S1743921318008220",
language = "English",
pages = "230--231",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",

}

RIS

TY - JOUR

T1 - Resonant multi-lane patterns in circumbinary young debris disks

AU - Demidova, Tatiana V.

AU - Shevchenko, Ivan I.

PY - 2020/1/1

Y1 - 2020/1/1

N2 - 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).

AB - 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).

KW - Methods: N-body simulations

KW - planetary systems: Protoplanetary disks

UR - http://www.scopus.com/inward/record.url?scp=85077898639&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/1104db8a-51ff-3942-984c-b9bc64d6509a/

U2 - 10.1017/S1743921318008220

DO - 10.1017/S1743921318008220

M3 - Article

AN - SCOPUS:85077898639

SP - 230

EP - 231

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -

ID: 53086675