Chemical evolution of galaxies in the high redshift universe

In this work, we present preliminary results on the chemical evolution of galaxies at 3 < z < 7 in cosmological simulations. The simulated mass-metallicity relation (MZR) predicted by the adopted supernova (SN) feedback model is consistent with recent observations. However, our findings sugges...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	De Rossi, M.E., Tissera, P.B.
Formato:	CONF
Materias:	Chemical abundances Cosmology Galaxy formation High redshift
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0094243X_v1294_n_p279_DeRossi
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Chemical evolution of galaxies in the high redshift universe
Publicado: (2010)

The mass-metallicity-kinematics relation of the stellar components of eagle galaxies
por: Zenocratti, Lucas José, et al.
Publicado: (2021)

Correlations between mass, stellar kinematics, and gas metallicity in EAGLE galaxies
por: Zenocratti, Lucas José, et al.
Publicado: (2020)

Chemical evolution of milky way type galaxies in the millennium simulation
por: De Rossi, M.E., et al.

The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
por: De Rossi, M.E., et al.

The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
Publicado: (2015)

Chemical enrichment at high redshifts: Understanding the nature of damped Lyα systems in hierarchical models
por: Tissera, P.B., et al.

Chemical signatures of formation processes in the stellar populations of simulated galaxies
por: Tissera, P.B., et al.

The Far-infrared Emission of the First Massive Galaxies
por: De Rossi, M.E., et al.

Chemical evolution of milky way type galaxies in the millennium simulation
Publicado: (2009)

The Far-infrared Emission of the First Massive Galaxies
Publicado: (2018)

Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations
por: Artale, M.C., et al.

Mild evolution of the stellar metallicity gradients of disc galaxies
por: Tissera, P.B., et al.

Milky Way type galaxies in a ΛcDM cosmology
por: De Rossi, M.E., et al.

A bias in optical observations of high-redshift luminous infrared galaxies
Publicado: (2004)

A bias in optical observations of high-redshift luminous infrared galaxies
por: Charmandaris, V., et al.

Chemical evolution during gas-rich galaxy interactions
por: Perez, J., et al.

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)

Chemical signatures of formation processes in the stellar populations of simulated galaxies
Publicado: (2012)

Effects of galaxy interactions in different environments
por: Sol Alonso, M., et al.

Effects of supernova feedback on the formation of galaxy discs
por: Scannapieco, C., et al.

Mild evolution of the stellar metallicity gradients of disc galaxies
Publicado: (2017)

Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations
Publicado: (2015)

Clues for the origin of the fundamental metallicity relations - I. The hierarchical building up of the structure
por: De Rossi, M.E., et al.

Chemical evolution using smooth particle hydrodynamical cosmological simulations - I. Implementation, tests and first results
por: Mosconi, M.B., et al.

Effects of galaxy interactions in different environments
Publicado: (2006)

The effects of galactic winds on the chemical evolution of baryons
por: De Rossi, M.E., et al.

A project to constrain emission from giant gaseous shells around high redshift radio galaxies
por: Moyano, Martín Manuel, et al.
Publicado: (2022)

A project to constrain emission from giant gaseous shells around high redshift radio galaxies
por: Moyano, Martín Manuel, et al.
Publicado: (2022)

Chemical evolution during gas-rich galaxy interactions
por: Perez, María Josefa, et al.
Publicado: (2011)

Milky Way type galaxies in a ΛcDM cosmology
Publicado: (2009)

Chemical evolution during gas-rich galaxy interactions
Publicado: (2011)

Connection between the star formation activity and stellar metallicities of galaxies in cosmological simulations
por: Grimozzi, Salvador, et al.
Publicado: (2022)

Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations - I. A model for chemical enrichment
por: Scannapieco, C., et al.

Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation
por: Tissera, P.B., et al.

Galaxy metallicity scaling relations in the EAGLE simulations
por: De Rossi, M.E., et al.

The stellar metallicity gradients in galaxy discs in a cosmological scenario
por: Tissera, P.B., et al.

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.

Effects of supernova feedback on the formation of galaxy discs
Publicado: (2008)