Formation of a two-dense-rings-pattern disk from the collapse of a cloud
In this paper, the formation of a disk resulting from the collapse of a rigidlyrotating cloud is studied. The plane perpendicular to the angular velocity axis that contains the star is the locus where materials falling from both sides face each other with the consequent formation of a double layer s...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2007
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57143203 |
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