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The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation

Rosen, Anna L; Krumholz, Mark


Stellar feedback in the form of radiation pressure and magnetically driven collimated outflows may limit the maximum mass that a star can achieve and affect the star formation efficiency of massive prestellar cores. Here we present a series of 3D adaptive mesh refinement radiation-magnetohydrodynamic simulations of the collapse of initially turbulent, massive prestellar cores. Our simulations include radiative feedback from both the direct stellar and dust-reprocessed radiation fields, and...[Show more]

CollectionsANU Research Publications
Date published: 2020
Type: Journal article
Source: The Astronomical Journal
DOI: 10.3847/1538-3881/ab9abf
Access Rights: Open Access


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