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Planet migration in accretion discs in binary systemsстатья
- Авторы: Nekrasov A.D., Popov S.B., Zhuravlev V.V.
- Журнал: Proceedings of the International Astronomical Union
- Том: 17
- Номер: S370
- Год издания: 2023
- Первая страница: 285
- Последняя страница: 286
- DOI: 10.1017/s174392132200388x
- Аннотация: We model evolution of exoplanets of S-type in close binary systems at the stage when the companion starts to lose mass via a slow stellar wind. At this stage an accretion disc is formed around the planets’ host. Detailed structure of such discs is calculated in quasi-stationary and non-stationary approaches. We model migration of planets embedded in these discs.
- Добавил в систему: Попов Сергей Борисович