Protostellar Disk Formation and Angular Momentum Transport During Magnetized Core Collapse - Archive ouverte HAL
Communication Dans Un Congrès Année : 2014

Protostellar Disk Formation and Angular Momentum Transport During Magnetized Core Collapse

Résumé

Theoretical studies of collapsing clouds have found that even a relatively weak magnetic field may prevent the formation of disks and their fragmentation. However, most previous studies have been limited to cases where the magnetic field and the rotation axis of the cloud are aligned, and very few studies investigated the combined effects of magnetic field and turbulence.
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Dates et versions

hal-03743168 , version 1 (02-08-2022)

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Marc Joos, Patrick Hennebelle, Andrea Ciardi. Protostellar Disk Formation and Angular Momentum Transport During Magnetized Core Collapse. The Labyrinth of Star Formation, 2014, Chania, Crete, Greece. pp.69, ⟨10.1007/978-3-319-03041-8_12⟩. ⟨hal-03743168⟩
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