FITTING PHOTOIONIZATION MODELS TO PLANETARY NEBULAE
Good to excellent photoionization models based on the Cloudy code were obtained for 13 out of 19 spectra of planetary nebulae. The two most important assumptions are that the photoionizing continuum is a Rauch model star, with gravity set by the condition that the stellar mass must be 1 M, and dens...
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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2009
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57115758016 |
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