The relation between the mass accretion rate and the disk mass in Class I Protostars

Author(s):
Fiorellino, E.; Tychoniec, Ł.; Manara, C.F.; Rosotti, G.P. (0000-0003-4853-5736); Antoniucci, S.; Miera, F.C.-S. de; Kóspál, Á.; Nisini, B.
Published
2022
Publication type
Article / Letter to editor
Star formationStellar accretion disksProtostarsLow mass starsPlanet formationCircumstellar disksCircumstellar dust15691579130220501241235236Astrophysics - Solar and Stellar Astrophysics
Date issued
2022
Language
English
Is part of
Astrophysical Journal Letters (2022), No. 1, L9
hdl
1887/3561742
doi
10.3847/2041-8213/ac8fee
URL
https://ui.adsabs.harvard.edu/abs/2022ApJ...937L...9F