Stellar multiplicity affects the correlation between protoplanetary disc masses and accretion rates: binaries explain high accretors in Upper Sco

Author(s):
Zagaria, F.; Clarke, C.J.; Rosotti, G.P. (0000-0003-4853-5736); Manara, C.F.
Published
2022
Publication type
Article / Letter to editor
accretionaccretion discsmethods miscellaneousplanets and satellites formationprotoplanetary discsbinaries closesubmillimetre planetary systemsAstrophysics - Solar and Stellar AstrophysicsAstrophysics - Earth and Planetary AstrophysicsAstrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 512, no. 3, p. 3538-3550
hdl
1887/3561756
doi
10.1093/mnras/stac621
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.512.3538Z