On dust evolution in planet-forming discs in binary systems: II. Comparison with Taurus and ρ Ophiuchus (sub-)millimetre observations: discs in binaries have small dust sizes

Author(s):
Zagaria, F.; Rosotti, G.P. (0000-0003-4853-5736); Lodato, G.
Published
2021
Publication type
Article / Letter to editor
AccretionAccretion discsOpacityPlanets and satellites: formationProtoplanetary discsBinaries: generalCircumstellar matterSubmillimetre: planetary systemsAstrophysics - 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. 507, no. 2, p. 2531-2549
hdl
1887/3275510
doi
10.1093/mnras/stab2024
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.2531Z