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Planet migration in accretion discs in binary systems
Published online by Cambridge University Press: 16 August 2023
Abstract
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.
- Type
- Poster Paper
- Information
- Proceedings of the International Astronomical Union , Volume 17 , Symposium S370: Winds of Stars and Exoplanets , August 2021 , pp. 285 - 286
- Copyright
- © The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union