Statistical analysis of molecular line emission from T tauri disk models
In this work we model the expected emission from the molecular lineC17O(J=3!2) in protoplanetary disks, modifying different physical parameters to obtain distinctive observational signatures. Our aim is to determine the kind of observations that will allow us to extract information about the physica...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2007
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57143204 |
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