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

T. V. Demidova, I. I. Shevchenko

Результат исследований: Научные публикации в периодических изданияхстатья

1 цитирование (Scopus)

Выдержка

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.

Язык оригиналаанглийский
Страницы (с-по)119-125
Число страниц7
ЖурналAstronomy Letters
Том44
Номер выпуска2
DOI
СостояниеОпубликовано - 1 фев 2018

Отпечаток

debris
planets
planet
protoplanets
planetesimal
binary stars
simulation
rings
ring structures
retaining
eccentricity
dust
orbitals

Предметные области Scopus

  • Астрономия и астрофизика
  • Космические науки и планетоведение

Цитировать

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Simulations of the Dynamics of the Debris Disks in the Systems Kepler-16, Kepler-34, and Kepler-35. / Demidova, T. V.; Shevchenko, I. I.

В: Astronomy Letters, Том 44, № 2, 01.02.2018, стр. 119-125.

Результат исследований: Научные публикации в периодических изданияхстатья

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