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High velocity outflows in quasars
Active Galactic Nuclei (AGN) are believedto be powered by accretion onto a Super-Massive Black Hole (SMBH). In order tohave material falling into the SMBH, angularmomentum conservation requires a counter-part for this accretion that is fueling theSMBH in the AGN. Outows might play anessential role i...
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| Izdano u: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Glavni autori: | , , |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2007
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| Teme: | |
| Online pristup: | https://www.redalyc.org/articulo.oa?id=57102974 |
| Oznake: |
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