Chemical Abundances and the Hierarchical Clustering

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dc.creatorTissera, Patricia B.
dc.creatorLambas, Diego G.
dc.date2003-10-20
dc.date.accessioned2026-07-07T02:10:39Z
dc.date.available2026-07-07T02:10:39Z
dc.descriptionWe studied 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 detail modeling of chemical enrichment by SNIa and SNII. In our simulations the metal missing problem is caused by chemical elements being locked upon in the central regions (or bulges) mainly, in stars. Supernova energy feedback could help to reduce this concentration by expelling metals to the intergalactic medium.
dc.descriptionto appear in Recycling intergalactic and intersetellar matter, IAUSS Vol 217, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0310559
dc.identifierhttp://arxiv.org/abs/astro-ph/0310559
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6808
dc.subjectAstrophysics
dc.titleChemical Abundances and the Hierarchical Clustering
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