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...
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
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| Kaituhi matua: | |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2007
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57143203 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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