The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies
Fuente:
Redalyc
Enregistré dans:
| Auteur principal: | |
|---|---|
| Format: | Artículo científico |
| Langue: | en |
| Publié: |
Universidad Nacional Autónoma de México
2002
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
| _version_ | 1876474049280868352 |
|---|---|
| author | A. Peimbert |
| author_facet | A. Peimbert |
| contents | The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies A. Peimbert M. Peimbert Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE GALAXIES: EVOLUTION GALAXIES: ABUNDANCES A few results that indicate the presence of temperature variations in gaseousnebulae are reviewed. The evidence is based on: a) temperatures derived fromdi erent methods, and b) on comparisons of abundances predicted by models ofgalactic chemical evolution with abundances derived from observations. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101427 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.14 |
| format | Artículo científico |
| id | redalyc_57101427 |
| institution | Redalyc |
| language | en |
| publishDate | 2002 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies A. Peimbert Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE GALAXIES: EVOLUTION GALAXIES: ABUNDANCES The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies A. Peimbert M. Peimbert Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE GALAXIES: EVOLUTION GALAXIES: ABUNDANCES A few results that indicate the presence of temperature variations in gaseousnebulae are reviewed. The evidence is based on: a) temperatures derived fromdi erent methods, and b) on comparisons of abundances predicted by models ofgalactic chemical evolution with abundances derived from observations. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101427 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.14 |
| title | The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies |
| topic | Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE GALAXIES: EVOLUTION GALAXIES: ABUNDANCES |
| url | https://www.redalyc.org/articulo.oa?id=57101427 |