MOLECULAR OBSERVATIONS OF THE ENVIRONS OF THE OXYGEN W-R STAR WR 102
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| Formato: | Artículo científico |
| Lenguaje: | en |
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Universidad Nacional Autónoma de México
2008
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| _version_ | 1876428537064325120 |
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| author | E. M. Arnal |
| author_facet | E. M. Arnal |
| contents | MOLECULAR OBSERVATIONS OF THE ENVIRONS OF THE OXYGEN W-R STAR WR 102 E. M. Arnal Física, Astronomía y Matemáticas type H II regions stars: early ISM: ionization models ISM: individual (M 43) We present the first results of a project aimed at the combined study of massive stars and their surrounding nebulae by means of a detailed study of Galactic Hii regions ionized by only one massive star. With this, we intend to check the validity of the new generation of massive star model atmosphere codes in terms of ionizing ux distribution. We take into account the efect of the nebular density distribution in our analyses. Various types of stellar and nebular observations have been collected for this purpose. 2008 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57116159049 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.33 |
| format | Artículo científico |
| id | redalyc_57116159049 |
| institution | Redalyc |
| language | en |
| publishDate | 2008 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | MOLECULAR OBSERVATIONS OF THE ENVIRONS OF THE OXYGEN W-R STAR WR 102 E. M. Arnal Física, Astronomía y Matemáticas type H II regions stars: early ISM: ionization models ISM: individual (M 43) MOLECULAR OBSERVATIONS OF THE ENVIRONS OF THE OXYGEN W-R STAR WR 102 E. M. Arnal Física, Astronomía y Matemáticas type H II regions stars: early ISM: ionization models ISM: individual (M 43) We present the first results of a project aimed at the combined study of massive stars and their surrounding nebulae by means of a detailed study of Galactic Hii regions ionized by only one massive star. With this, we intend to check the validity of the new generation of massive star model atmosphere codes in terms of ionizing ux distribution. We take into account the efect of the nebular density distribution in our analyses. Various types of stellar and nebular observations have been collected for this purpose. 2008 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57116159049 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.33 |
| title | MOLECULAR OBSERVATIONS OF THE ENVIRONS OF THE OXYGEN W-R STAR WR 102 |
| topic | Física, Astronomía y Matemáticas type H II regions stars: early ISM: ionization models ISM: individual (M 43) |
| url | https://www.redalyc.org/articulo.oa?id=57116159049 |