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| Format: | Artículo científico |
| Language: | en |
| Published: |
Universidad Nacional Autónoma de México
2001
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| Online Access: | https://www.redalyc.org/articulo.oa?id=57101034 |
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| _version_ | 1866815620005232640 |
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| author | Antonio Peimbert |
| author_facet | Antonio Peimbert |
| contents | Primordial helium abundance determinations Antonio Peimbert Manuel Peimbert Valentina Luridiana Física, Astronomía y Matemáticas GALAXIES: ISM H II REGIONS ISM: ABUNDANCES GALAXIES: ABUNDANCES Based on the best observations of extragalactic H ii regions of low metal-licity available in the literature we redetermine the primordial helium abundance,Yp, taking into account all the observed He i line intensities with the exceptionof those strongly a ected by underlying absorption. We derive He/H, Ne(He ii),Te(He ii), and (3889) self{consistently. We present results for NGC 346, I Zw 18,and NGC 2363. From these objects we nd that Yp = 0:2351 0:0022. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101034 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.10 |
| format | Artículo científico |
| id | redalyc_57101034 |
| language | en |
| publishDate | 2001 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Primordial helium abundance determinations Antonio Peimbert Física, Astronomía y Matemáticas GALAXIES: ISM H II REGIONS ISM: ABUNDANCES GALAXIES: ABUNDANCES Primordial helium abundance determinations Antonio Peimbert Manuel Peimbert Valentina Luridiana Física, Astronomía y Matemáticas GALAXIES: ISM H II REGIONS ISM: ABUNDANCES GALAXIES: ABUNDANCES Based on the best observations of extragalactic H ii regions of low metal-licity available in the literature we redetermine the primordial helium abundance,Yp, taking into account all the observed He i line intensities with the exceptionof those strongly a ected by underlying absorption. We derive He/H, Ne(He ii),Te(He ii), and (3889) self{consistently. We present results for NGC 346, I Zw 18,and NGC 2363. From these objects we nd that Yp = 0:2351 0:0022. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101034 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.10 |
| title | Primordial helium abundance determinations |
| topic | Física, Astronomía y Matemáticas GALAXIES: ISM H II REGIONS ISM: ABUNDANCES GALAXIES: ABUNDANCES |
| url | https://www.redalyc.org/articulo.oa?id=57101034 |