Photoionization and shock modelling of the h II region abundance sequence and of luminous infrared galaxies
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| Format: | Artículo científico |
| Sprache: | en |
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Universidad Nacional Autónoma de México
2000
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| _version_ | 1876477227682496512 |
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| author | L. J. Kewley |
| author_facet | L. J. Kewley |
| contents | Photoionization and shock modelling of the h II region abundance sequence and of luminous infrared galaxies L. J. Kewley M. A. Dopita C. A. Heisler R. S. Sutherland B. Rocca Volmerange E. Moy Física, Astronomía y Matemáticas H II REGIONS GALAXIES: ISM GALAXIES: STARBURST GALAXIES: ABUNDANCES We recalibrate the abundance sequence for extragalactic H II regions andcompare photoionization and shock models for a luminous sub-sample of southernstarburst galaxies. We nd H II regions are young. Luminous IR galaxies are excitedby continuous star formation and/or AGN and have higher than solar metallicity. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100940 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.9 |
| format | Artículo científico |
| id | redalyc_57100940 |
| institution | Redalyc |
| language | en |
| publishDate | 2000 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Photoionization and shock modelling of the h II region abundance sequence and of luminous infrared galaxies L. J. Kewley Física, Astronomía y Matemáticas H II REGIONS GALAXIES: ISM GALAXIES: STARBURST GALAXIES: ABUNDANCES Photoionization and shock modelling of the h II region abundance sequence and of luminous infrared galaxies L. J. Kewley M. A. Dopita C. A. Heisler R. S. Sutherland B. Rocca Volmerange E. Moy Física, Astronomía y Matemáticas H II REGIONS GALAXIES: ISM GALAXIES: STARBURST GALAXIES: ABUNDANCES We recalibrate the abundance sequence for extragalactic H II regions andcompare photoionization and shock models for a luminous sub-sample of southernstarburst galaxies. We nd H II regions are young. Luminous IR galaxies are excitedby continuous star formation and/or AGN and have higher than solar metallicity. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100940 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.9 |
| title | Photoionization and shock modelling of the h II region abundance sequence and of luminous infrared galaxies |
| topic | Física, Astronomía y Matemáticas H II REGIONS GALAXIES: ISM GALAXIES: STARBURST GALAXIES: ABUNDANCES |
| url | https://www.redalyc.org/articulo.oa?id=57100940 |