Protostellar Disk Formation and Angular Momentum Transport During Magnetized Core Collapse

Joos, Marc; Hennebelle, P.; Ciardi, A.

doi:10.1007/978-3-319-03041-8_12

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2017

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“…In those cases, a flattened envelope (that is, pseudodisk), but not a large rotationally supported disk, can form around the central source (9). A misalignment between the magnetic field and the axis of rotation ( 10 , 11 ) and the nonideal magnetohydrodynamic (MHD) effects ( 12 ) can sometimes solve this catastrophe. Even when a disk is formed, if a significant fraction of the magnetic flux of the dense core is dragged into it, the disk would rotate at a sub-Keplerian speed because of magnetic support ( 13 ).…”

Section: Introductionmentioning

confidence: 99%