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Chemical Evolution in Hierarchical Clustering Scenarios

Published online by Cambridge University Press:  26 May 2016

Patricia B. Tissera  and
Cecilia Scannapieco
Patricia B. Tissera
Affiliation:
Institute of Astronomy and Space Physics, CONICET, Argentina
Cecilia Scannapieco
Affiliation:
Institute of Astronomy and Space Physics, CONICET, Argentina

Abstract

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We present first results of an implementation of chemical evolution in a cosmological hydrodynamical code, focusing the analysis on the effects of cooling baryons according to their metallicity. We found that simulations with primordial cooling can underestimate the star formation rate from z < 3 and by up to ≈ 20%. We constructed simulated spectra by combining the star formation and chemical history of galactic systems with spectral synthesis models and assess the impact of chemical evolution on the energy distribution.

Type
Part 2. Origin
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 258 - 263
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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