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The relation between the Mass Accretion Rate and the Disk Mass in Class I Protostars

By Eleonora Fiorellino and others
The evidence of a relation between the mass accretion rate and the disk mass is established for young, Class II pre-main sequence stars. This observational result opened an avenue to test theoretical models and constrain the initial conditions of the disk formation, fundamental in the understanding of the emergence of... Show more
September 9, 2022
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The relation between the Mass Accretion Rate and the Disk Mass in Class I Protostars
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