Planet formation in a disk around a star: The two dense-ring model
A disk around a star is the initial configuration commonly accepted for the material that forms a planetary system such as our own. In this work, the first stage in the evolution from a disk to a set of planetesimals is studied. This stage consists in the formation ofdense regions, which are able to...
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| Pubblicato in: | Revista Mexicana de Ciencias Geológicas |
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| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2010
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57216002011 |
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