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The Effects of Galactic Winds on the Chemical Evolution of Baryons

Published online by Cambridge University Press:  13 April 2010

María E. De Rossi  and
Patricia B. Tissera
María E. De Rossi
Affiliation:
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC67 Suc28, Ciudad Autónoma de Buenos Aires (1428), Argentina email: [email protected] Consejo Nacional de Investigaciones Científicas y Técnicas, Rivadavia 1917, Ciudad Autónoma de Buenos Aires (1428), Argentina
Patricia B. Tissera
Affiliation:
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC67 Suc28, Ciudad Autónoma de Buenos Aires (1428), Argentina email: [email protected] Consejo Nacional de Investigaciones Científicas y Técnicas, Rivadavia 1917, Ciudad Autónoma de Buenos Aires (1428), Argentina
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Abstract

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During the last decade, the development of more sophisticated surveys allows the exploration of the chemical enrichment of galaxies and their environment at different cosmic times. In this context, it has been suggested that galactic winds play a fundamental role in the regulation of the star formation and the transportation of metals outside the galaxies. In this work, we study the influence of Supernovae winds in the chemical evolution of galaxies and the intergalactic medium by employing cosmological numerical simulations within a hierarchical Universe. We focus on the origin and evolution of the mass-metallicity relation (MZR).

Keywords

Galaxies: formationGalaxies: evolutionCosmology: dark matter
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 325 - 326
Copyright
Copyright © International Astronomical Union 2010

References

de Rossi, M. E., Tissera, P. B., & Scannapieco, C. 2007, MNRAS, 374, 323Google Scholar
Erb, D. K., et al. 2006, ApJ, 646, 107Google Scholar
Maiolino, R., et al. 2008, A&A, 488, 463Google Scholar
Scannapieco, C., Tissera, P. B., White, S. D. M., & Springel, V. 2006, MNRAS, 371, 1125CrossRefGoogle Scholar
Springel, V., White, S. D. M., Tormen, G., & Kauffmann, G. 2001, MNRAS, 328, 726CrossRefGoogle Scholar
Tissera, P. B., De Rossi, M. E., & Scannapieco, C. 2005, MNRAS, 364, L38Google Scholar
Tremonti, C., et al. 2004, ApJ, 613, 898Google Scholar
Zhang, W., et al. 2009, MNRAS, 397, 1243CrossRefGoogle Scholar