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.
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2000 |
| País: | México |
| Institución: | Universidad Nacional Autónoma de México |
| Repositorio: | Redalyc-UNAM |
| OAI Identifier: | oai:redalyc.org:57100956 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57100956 |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas H II REGIONS ISM: INDIVID DUST: EXTINCTION UAL (ORION NEBULA) |
| Sumario: | 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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