On dust evolution in planet-forming discs in binary systems: I. Theoretical and numerical modelling: radial drift is faster in binary discs

Author(s):
Zagaria, F.; Rosotti, G.P. (0000-0003-4853-5736); Lodato, G.
Published
2021
Publication type
Article / Letter to editor
AccretionAccretion discsMethods: numericalPlanets and satellites: formationProtoplanetary discsBinaries: generalCircumstellar matterAstrophysics - Earth and planetary astrophysicsAstrophysics - solar and stellar astrophysics
Date issued
2021
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2021), Vol. 504, no. 2, p. 2235-2252
hdl
1887/3275817
doi
10.1093/mnras/stab985
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.504.2235Z