MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus

Author(s):
Tabone, B.X.J.A.; Rosotti, G.P. (0000-0003-4853-5736); Lodato, G.; Armitage, P.J.; Cridland, A.J.; Dishoeck, E.F. van (0000-0001-7591-1907)
Published
2022
Publication type
Article / Letter to editor
Accretion DiscsMHD Disc WindsProtoplanetary DiscsSubmillimetre: Planetary SystemsAstrophysics - Earth and Planetary AstrophysicsAstrophysics - Astrophysics of GalaxiesAstrophysics - Solar and Stellar Astrophysics
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society: Letters (2022), Vol. 512, no. 1, p. L74-L79
hdl
1887/3264038
doi
10.1093/mnrasl/slab124
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.tmpL.109T