CHEMICAL ABUNDANCES AND GAS CONTENT IN DISK GALAXIES: CORRELATIONS WITH THE X SPIN PARAMETER
By using a very simple and general model to describe the dynamics of disk galaxies, we estimate the L spin parameter for a sample of observed galaxies and present a study in which we show that several important physical properties are intrinsically related to the dynamics of the systems. Although co...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2009
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57112288005 |
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