The Chemical Evolution of Narrow Emission Line Galaxies: the Key to their Formation Processes
Using the largest sample of narrow emission line galaxies available so far, we show that their spectral characteristics are correlated with different physical parameters, like the chemical abundances, the morphologies, the masses of the bulge and the mean stellar age of the stellar populations of th...
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| Vydáno v: | Acta Universitaria |
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| Hlavní autoři: | , , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad de Guanajuato
2011
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=41620852011 |
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