Disk wind
In astronomy, a disk wind is a particle outflow observed around accretion disks, mainly near protoplanetary disks and active galactic nuclei (AGN). The disk wind is made up of a gaseous and a dusty component.
In astronomy, a disk wind is a particle outflow observed around accretion disks, mainly near protoplanetary disks and active galactic nuclei (AGN). The disk wind is made up of a gaseous and a dusty component.
In astronomy, a disk wind is a particle outflow observed around accretion disks, mainly near protoplanetary disks and active galactic nuclei (AGN). The disk wind is made up of a gaseous and a dusty component.
Source: Wikipedia "Disk wind" · CC BY-SA 4.0
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