Chemical Enrichment at High Redshifts: Understanding the Nature of Damped Lyα Systems in Hierarchical Models

We use cosmological hydrodynamical simulations including star formation and metal enrichment to study the evolution of the chemical properties of galaxy-like objects at high redshift in the range 0.25 < z < 2.35 in a hierarchical clustering scenario. We find that as the galactic objects are as...

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Detalles Bibliográficos
Autores principales:	Tissera, Patricia Beatriz, García Lambas, Diego Rodolfo, Mosconi, Mirta B., Cora, Sofía Alejandra
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2001
Materias:	Astronomía cosmology: theory dark matter galaxies: abundances galaxies: evolution galaxies: formation methods: numerical
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/101546 https://ri.conicet.gov.ar/11336/22485 http://iopscience.iop.org/article/10.1086/321672
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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