The Relation between the Mass Accretion Rate and the Disk Mass in Class I Protostars (2022)

First Author: Fiorellino E
Attributed to:  Connecting theories and observations of planet formation funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/2041-8213/ac8fee

Publication URI: http://dx.doi.org/10.3847/2041-8213/ac8fee

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal Letters

Issue: 1