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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. Especially in edge-on protoplanetary disks this disk wind can be directly imaged.
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disk wind winds accretion protoplanetary disks around mhd stellar objects lines star material jets photons also active galactic nuclei region
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Disk wind | is a | particle outflow observed around accretion disks | 0.90 | text |
| Disk wind | is a | major contributor to accretion in young stellar objects | 0.90 | text |
| Disk wind | related to Active galactic nuclei | Outflows | 0.60 | section |
| Disk wind | related to Active galactic nuclei | SMBH | 0.60 | section |
| Disk wind | related to Active galactic nuclei | These | 0.60 | section |
| Disk wind | related to Active galactic nuclei | AGN | 0.60 | section |
| Disk wind | related to Active galactic nuclei | BALQSOs | 0.60 | section |
| Disk wind | related to Active galactic nuclei | Several | 0.60 | section |
| Disk wind | related to Active galactic nuclei | One | 0.60 | section |
| Disk wind | related to Active galactic nuclei | In | 0.60 | section |
| Disk wind | related to Active galactic nuclei | UV | 0.60 | section |
| Disk wind | related to Active galactic nuclei | Many | 0.60 | section |
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