The Mass Accretion Rate and Stellar Properties in Class I Protostars

The Mass Accretion Rate and Stellar Properties in Class I Protostars

Stars collect most of their mass during the protostellar stage, yet the accretion luminosity and stellar parameters, which are needed to compute the mass accretion rate, are poorly constrained for the youngest sources. The aim of this work is to fill this gap, computing the stellar properties and th...

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Bibliographic Details
Main Authors: Eleonora Fiorellino, Łukasz Tychoniec, Fernando Cruz-Sáenz de Miera, Simone Antoniucci, Ágnes Kóspál, Carlo F. Manara, Brunella Nisini, Giovanni Rosotti
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Star formation
Stellar accretion disks
Stellar properties
Protostars
Low mass stars
Circumstellar disks
Online Access:https://doi.org/10.3847/1538-4357/aca320

Internet

https://doi.org/10.3847/1538-4357/aca320

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