A HYDRODYNAMICAL MECHANISM FOR GENERATING ASTROPHYSICAL JETS
Whenever in a classical accretion disk the thin disk approximation fails inte- rior to a certain radius, a transition from Keplerian to radial infalling trajectories should occur. We show that this transition is actually expected to occur inte- rior to a certain critical radius, provided surface den...
Gorde:
| Argitaratua izan da: | Revista Mexicana de Astronomía y Astrofísica |
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| Egile Nagusiak: | , , , |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2014
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| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=57131044004 |
| Etiketak: |
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