Modelling the secular evolution of protoplanetary disc dust sizes: a comparison between the viscous and magnetic wind case

Author(s):
Zagaria, F.; Rosotti, G.P. (0000-0003-4853-5736); Clarke, C.J.; Tabone, B.
Published
2022
Publication type
Article / Letter to editor
accretionaccretion discsMHDmethods numericalplanets and satellites formationprotoplanetary discssubmillimetre planetary systemsAstrophysics - Earth and Planetary AstrophysicsAstrophysics - Solar and Stellar Astrophysics
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 514, no. 1, p. 1088-1106
hdl
1887/3561750
doi
10.1093/mnras/stac1461
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.514.1088Z