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.
Furkejuvvon:
| Publikašuvnnas: | Revista Mexicana de Astronomía y Astrofísica |
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| Váldodahkkit: | , , |
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Universidad Nacional Autónoma de México
2001
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| Fáttát: | |
| Liŋkkat: | https://www.redalyc.org/articulo.oa?id=57101010 |
| Fáddágilkorat: |
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