arXiv
Open Access
2019
Simulations of the dynamics of the debris disks in the systems Kepler-16, Kepler-34, and Kepler-35
Tatiana Demidova
Ivan Shevchenko
Abstrak
The long-term dynamics of planetesimals in debris discs in models with parameters of binary star systems Kepler-16, Kepler-34 and Kepler-35 with planets is investigated. Our calculations have shown the formation of a stable coorbital with the planet ring is possible for Kepler-16 and Kepler-35 systems. In Kepler-34 system, significant eccentricities of the orbits of the binary and planets can to prevent the formation of such a structure. Detection circumbinary annular structures in observations of systems binary stars can be evidence of the existence of planets, retaining coorbital rings from dust and planetesimals.
Topik & Kata Kunci
Penulis (2)
T
Tatiana Demidova
I
Ivan Shevchenko
Akses Cepat
Informasi Jurnal
- Tahun Terbit
- 2019
- Bahasa
- en
- Sumber Database
- arXiv
- Akses
- Open Access ✓