MAPPING AND MODELING THE PROPERTIES OF BIPOLAR PLANETARY NEBULAE
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| Format: | Artículo científico |
| Language: | en |
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Universidad Nacional Autónoma de México
2011
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| _version_ | 1876456383629492224 |
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| author | D. M. Faes |
| author_facet | D. M. Faes |
| contents | MAPPING AND MODELING THE PROPERTIES OF BIPOLAR PLANETARY NEBULAE D. M. Faes R. D. D. Costa C. Morisset Física, Astronomía y Matemáticas Methods numerical NGC 6572) planetary nebulae individual (IC 4406 We present the first results of a project aimed to derive physical parameters, chemical abundances and angular variations of spatially resolved planetary nebulae in the Galaxy that have bipolar structure. These results can be used as input and constraints into numerical simulations in order to reproduce their properties in the visual band of the spectrum. This provides a way to examine the non-homogeneity present in this kind of object, as well as a tool to derive their intrinsic properties, like tridimensional geometry and matter distribution, central star properties, distance, and other properties in a self-consistent way. Here we show our findings for two of these objects: IC 4406 and NGC 6572. 2011 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57121297119 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.40 |
| format | Artículo científico |
| id | redalyc_57121297119 |
| institution | Redalyc |
| language | en |
| publishDate | 2011 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | MAPPING AND MODELING THE PROPERTIES OF BIPOLAR PLANETARY NEBULAE D. M. Faes Física, Astronomía y Matemáticas Methods numerical NGC 6572) planetary nebulae individual (IC 4406 MAPPING AND MODELING THE PROPERTIES OF BIPOLAR PLANETARY NEBULAE D. M. Faes R. D. D. Costa C. Morisset Física, Astronomía y Matemáticas Methods numerical NGC 6572) planetary nebulae individual (IC 4406 We present the first results of a project aimed to derive physical parameters, chemical abundances and angular variations of spatially resolved planetary nebulae in the Galaxy that have bipolar structure. These results can be used as input and constraints into numerical simulations in order to reproduce their properties in the visual band of the spectrum. This provides a way to examine the non-homogeneity present in this kind of object, as well as a tool to derive their intrinsic properties, like tridimensional geometry and matter distribution, central star properties, distance, and other properties in a self-consistent way. Here we show our findings for two of these objects: IC 4406 and NGC 6572. 2011 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57121297119 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.40 |
| title | MAPPING AND MODELING THE PROPERTIES OF BIPOLAR PLANETARY NEBULAE |
| topic | Física, Astronomía y Matemáticas Methods numerical NGC 6572) planetary nebulae individual (IC 4406 |
| url | https://www.redalyc.org/articulo.oa?id=57121297119 |