Magnetic outflows from turbulent accretion disks: I. Vertical structure and secular evolution

Context. Astrophysical disks are likely embedded in an ambient vertical magnetic field generated by its environment. This ambient field is known to drive magneto-rotational turbulence in the disk bulk, but it is also responsible for launching magnetised outflows at the origin of astrophysical jets....

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-03, Vol.647, p.A192
Hauptverfasser:	Jacquemin-Ide, J., Lesur, G., Ferreira, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Physics
Online-Zugang:	Volltext
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