Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-21T08:11:31.021Z Has data issue: false hasContentIssue false
  • English
  • Français

Planet migration in accretion discs in binary systems

Published online by Cambridge University Press:  16 August 2023

A.D. Nekrasov ,
S.B. Popov Open the ORCID record for S.B. Popov [Opens in a new window]  and
V.V. Zhuravlev
A.D. Nekrasov
Affiliation:
Department of Physics, Lomonosov Moscow State University, 119991, Moscow, Russia Sternberg Astronomical Institute, 119234, Universitetski pr. 13, Moscow, Russia
S.B. Popov
Affiliation:
Department of Physics, Lomonosov Moscow State University, 119991, Moscow, Russia Sternberg Astronomical Institute, 119234, Universitetski pr. 13, Moscow, Russia
V.V. Zhuravlev
Affiliation:
Sternberg Astronomical Institute, 119234, Universitetski pr. 13, Moscow, Russia
Get access Rights & Permissions [Opens in a new window]

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.

Keywords

planetary systemsbinaries: closeaccretion disks
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S370: Winds of Stars and Exoplanets , August 2021 , pp. 285 - 286
Check for updates
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Kulikova, O, Popov, S. B., Zhuravlev, V. V., 2019, MNRAS, 487, 3069 10.1093/mnras/stz1363CrossRefGoogle Scholar
Paxton, O., Bildsten, L., Dotter, A., et al., 2011, ApJS, 192, 3 10.1088/0067-0049/192/1/3CrossRefGoogle Scholar
Supplementary material: PDF

Nekrasov et al. supplementary material

Nekrasov et al. supplementary material

Download Nekrasov et al. supplementary material(PDF)
PDF 683.5 KB