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...
Guardado en:
Autores principales: | Tissera, P.B., Lambas, D.G., Mosconi, M.B., Cora, S. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v557_n2PART1_p527_Tissera |
Aporte de: |
Ejemplares similares
-
Chemical Enrichment at High Redshifts: Understanding the Nature of Damped Lyα Systems in Hierarchical Models
por: Tissera, Patricia Beatriz, et al.
Publicado: (2001) -
Chemical enrichment at high redshifts: Understanding the nature of damped Lyα systems in hierarchical models
Publicado: (2001) -
Building blocks in hierarchical clustering scenarios and their connection with damped Lyα systems
por: Cora, Sofía Alejandra, et al.
Publicado: (2003) -
Nitrogen abundances in damped Lyman a systems: The combined effects of SNII and SNIa in a hierarchical clustering scenario
por: Tissera, P.B., et al. -
Nitrogen abundances in damped Lyman α systems: the combined effects of SNII and SNIa in a hierarchical clustering scenario
por: Tissera, Patricia Beatriz, et al.
Publicado: (2002)