The influence of turbulence during magnetized core collapse and its consequences on low-mass star formation

[Abridged] Theoretical and numerical studies of star formation have shown that magnetic field (B) has a strong influence on both disk formation and fragmentation; even a relatively low B can prevent these processes. However, very few studies investigated the combined effects of B and turbulence. We...

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Veröffentlicht in:	arXiv.org 2013-03
Hauptverfasser:	Joos, Marc, Hennebelle, Patrick, Ciardi, Andrea, Fromang, Sebastien
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular momentum Brake disks Braking Computer simulation Fragmentation Initial conditions Low mass stars Magnetic diffusion Magnetization Magnetohydrodynamic turbulence Misalignment Outflow Physics - Astrophysics of Galaxies Physics - Solar and Stellar Astrophysics Protostars Rotation Star & galaxy formation Star formation Turbulent diffusion Velocity distribution
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