Long-term stability of planets in and around binary stars

Autor: Richard D Smith, Tore Espaas, Harry A Ballantyne, Richard J. Parker, Bethan Z Norgrove, Isaac L Pepper, Rosie E Dommett, Benjamin R Harris, Bethany A Wootton

Publikováno v: Ballantyne, H A, Espaas, T, Norgrove, B Z, Wootton, B A, Harris, B R, Pepper, I L, Smith, R D, Dommett, R E & Parker, R J 2021, ' Long-term stability of planets in and around binary stars ', Monthly Notices of the Royal Astronomical Society, vol. 507, no. 3, pp. 4507-4520 . https://doi.org/10.1093/mnras/stab2324

Planets are observed to orbit the component star(s) of stellar binary systems on so-called circumprimary or circumsecondary orbits, as well as around the entire binary system on so-called circumbinary orbits. Depending on the orbital parameters of th

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1b39dd810117c54ac94bb9db5630817
https://doi.org/10.1093/mnras/stab2324