PLANETARY INFLUENCE IN THE GAP OF A PROTOPLANETARY DISK: STRUCTURE FORMATION AND AN APPLICATION TO V1247 ORI
We present a set of hydrodynamical models of a planetary system embedded in a protoplanetary disk in order to extract the number of dust structures formed in the disk, their masses and sizes, within optical depth range s τ ≤ 0 .5, 0 . 5 < τ<2 and τ ≥2. The study of the structures shows: (1) an incre...
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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2017
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57153206010 |
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