Gravitoturbulence in magnetized protostellar discs

Gravitational instability (GI) features in several aspects of protostellar disc evolution, most notably in angular momentum transport, fragmentation, and the outbursts exemplified by FU Ori and EX Lupi systems. The outer regions of protostellar discs may also be coupled to magnetic fields, which cou...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-08, Vol.460 (2), p.2223-2237
Hauptverfasser:	Riols, A., Latter, H.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astronomy Disks Fragmentation Gravitational instability Gravity Ionization Ions Magnetic fields Magnetism Protostars Simulation Stars & galaxies Symbols
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