| Texto completo | |
| Autor(es): |
Kirby, Evan N.
[1]
;
Lanfranchi, Gustavo A.
[2]
;
Simon, Joshua D.
[3]
;
Cohen, Judith G.
[1]
;
Guhathakurta, Puragra
[4]
Número total de Autores: 5
|
| Afiliação do(s) autor(es): | [1] CALTECH, Dept Astron, Pasadena, CA 91125 - USA
[2] Univ Cruzeiro Sul, Nucleo Astrofis Teor, BR-01506000 Sao Paulo - Brazil
[3] Observ Carnegie Inst Washington, Pasadena, CA 91101 - USA
[4] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Dept Astron & Astrophys, Santa Cruz, CA 95064 - USA
Número total de Afiliações: 4
|
| Tipo de documento: | Artigo Científico |
| Fonte: | ASTROPHYSICAL JOURNAL; v. 727, n. 2 FEB 1 2011. |
| Citações Web of Science: | 182 |
| Resumo | |
We present metallicity distribution functions (MDFs) for the central regions of eight dwarf satellite galaxies of the Milky Way: Fornax, Leo I and II, Sculptor, Sextans, Draco, Canes Venatici I, and Ursa Minor. We use the published catalog of abundance measurements from the previous paper in this series. The measurements are based on spectral synthesis of iron absorption lines. For each MDF, we determine maximum likelihood fits for Leaky Box, Pre-Enriched, and Extra Gas (wherein the gas supply available for star formation increases before it decreases to zero) analytic models of chemical evolution. Although the models are too simplistic to describe any MDF in detail, a Leaky Box starting from zero metallicity gas fits none of the galaxies except Canes Venatici I well. The MDFs of some galaxies, particularly the more luminous ones, strongly prefer the Extra Gas Model to the other models. Only for Canes Venatici I does the Pre-Enriched Model fit significantly better than the Extra Gas Model. The best-fit effective yields of the less luminous half of our galaxy sample do not exceed 0.02 Z(circle dot), indicating that gas outflow is important in the chemical evolution of the less luminous galaxies. We surmise that the ratio of the importance of gas infall to gas outflow increases with galaxy luminosity. Strong correlations of average {[}Fe/H] and metallicity spread with luminosity support this hypothesis. (AU) | |
| Processo FAPESP: | 06/57824-1 - Aplicação de modelos teórico-computacionais em Astrofísica |
| Beneficiário: | Gustavo Amaral Lanfranchi |
| Modalidade de apoio: | Auxílio à Pesquisa - Jovens Pesquisadores |