Dust and the temperature structure of orion
In this work two photoionization models were calculated: (a) with dust, (b)with high densities. We compared the models with a new long slit spectrum of theOrion Nebula.
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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
2000
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57100956 |
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