Resumen
The oxygen abundances of 18 dwarf spiral galaxies are presented. In most of them, the abundance are determined with semi empirical methods. We find that the values are sub-solar for most of the galaxies, similar to those observed in other late-type galaxies, as BCG or dwarf irregular. The abundance gradient can be determined in four of these galaxies, one of them a barred one. The gradients of the three non-barred galaxies in the sample are larger than-0.15 dex/kpc, while the gradient of the barred galaxy is shallower, only-0.1 dex/kpc.
Título traducido de la contribución | Abundancias químicas de las galaxias espirales enanas |
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Idioma original | Inglés |
Páginas (desde-hasta) | 60-61 |
Número de páginas | 2 |
Publicación | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volumen | 40 |
Estado | Publicada - 2011 |
Evento | 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010 - Morelia, Michoacan, México Duración: 8 nov. 2010 → 12 nov. 2010 |