Photoionization dusty models of the planetary nebula NGC 6302
Using photoionization calculations with dust, we model the high excitationinfrared lines of NGC 6302. This object is a high excitation bipolar planetarynebula of Peimbert type I. We nd that including the dust results in a signicantlyhotter nebula.
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2001 |
| País: | México |
| Institución: | Universidad Nacional Autónoma de México |
| Repositorio: | Redalyc-UNAM |
| OAI Identifier: | oai:redalyc.org:57101010 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57101010 |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas ISM:DUST ISM: PLANE INFRARED: ISM: LINES TARY NEBULAE: NGC 6302 |
| Sumario: | Using photoionization calculations with dust, we model the high excitationinfrared lines of NGC 6302. This object is a high excitation bipolar planetarynebula of Peimbert type I. We nd that including the dust results in a signicantlyhotter nebula. |
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