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Symposium - International Astronomical Union
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Symposium - International Astronomical Union
Article . 2004 . Peer-reviewed
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Chemical Abundances and Hierarchical Clustering

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 2004Publisher:Cambridge University Press (CUP)Journal:Symposium - International Astronomical Union, volume 217, pages 264-265 (issn: 0074-1809, Copyright policy )
Authors: D.G. Lambas; P. B. Tissera;

doi: 10.1017/s0074180900197682

Chemical Abundances and Hierarchical Clustering

Abstract

In this contribution we study the chemical enrichment of the interstellar medium and stellar population of the building blocks of current typical galaxies in the field, in cosmological hydrodynamics simulations. The simulations include detailed modeling of chemical enrichment by SNIa and SNII In our simulations the missing metal problem is caused by chemical elements being locked up in stars, in the central regions (or bulges) mainly. Supernova energy feedback could help to reduce this concentration by expelling metals to the intergalactic medium.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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