Insight into the physical processes that shape the metallicity profiles in galaxies

Los perfiles radiales de abundancia en galaxias son el resultado de interacciones complejas entre una variedad de procesos físicos tales como inflows/outflows de gas, SN/AGN feedback, interacciones o fusiones de galaxias, etc. Modelos simples de formación inside-out predicen un gradiente negativo en...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Tapia, B., Tissera, Patricia Beatriz, Sillero, E., Casanueva, C., Pedrosa, Susana Elizabeth, Bignone, Lucas Axel, Dominguez Tenreiro, Rosa María, Padilla, Nelson
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2022
Materias:	Ciencias Astronómicas galaxies: abundances galaxies: evolution methods: numerical
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/168656
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

Ejemplares similares

The gas metallicity gradient and the star formation activity of disc galaxies
por: Tissera, P.B., et al.

Connection between feedback processes and the effective yields of EAGLE galaxies
por: Zerbo, María Candela, et al.
Publicado: (2024)

Effective yields as tracers of feedback effects on the metal enrichment of galaxies
por: Zerbo, María Candela, et al.
Publicado: (2023)

Effects of feedback processes on the effective yields of galaxies
por: Zerbo, María Candela, et al.
Publicado: (2022)

Local metallicity in simulated galaxies
por: Collacchioni, Florencia, et al.
Publicado: (2021)

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

The mass-metallicity relation of interacting galaxies
por: Michel-Dansac, L., et al.

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

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

The mass-metallicity relation of interacting galaxies
Publicado: (2008)

The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
por: Collacchioni, Florencia, et al.
Publicado: (2020)

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

The gas metallicity gradient and the star formation activity of disc galaxies
Publicado: (2016)

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

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

New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
por: Castro, Cínthia S., et al.
Publicado: (2017)

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

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

The mass-metallicity relation: A fossil from the star formation history of galaxies
por: De Rossi, M.E.

The mass-metallicity relation: A fossil from the star formation history of galaxies
Publicado: (2012)

Chemical abundance patterns in Local Group galaxies within cosmological simulations
por: Biaus, L., et al.
Publicado: (2021)

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

Modelling satellite galaxies in semi-analytical models
por: Delfino, F. M., et al.
Publicado: (2021)

Chemical properties of galaxy baryons as a function of halo mass in a ΛCDM cosmology
por: Burrafato, Y. D., et al.
Publicado: (2024)

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

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

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

Chemical evolution using smooth particle hydrodynamical cosmological simulations - I. Implementation, tests and first results
por: Mosconi, M. B., et al.
Publicado: (2001)

Integral field spectroscopy of nitrogen overabundant blue compact dwarf galaxies
por: Pérez-Montero, E., et al.
Publicado: (2011)

Age and metallicity gradients in simulated galaxies of the Local Group
por: Marioni, O. F., et al.
Publicado: (2021)

Metallicity evolution of AGNs from UV emission lines based on a new index
por: Dors Jr., Oli L., et al.
Publicado: (2014)

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

Galaxy metallicity scaling relations in the EAGLE simulations
Publicado: (2017)

Analysing derived metallicities and ionization parameters from model-based determinations in ionized gaseous nebulae
por: Dors Junior, O. L., et al.
Publicado: (2011)

Gas accretion onto the disc of a simulated Milky Way-mass galaxy
por: Iza, F. G., et al.
Publicado: (2021)

Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation
Publicado: (2005)

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

The temporal evolution of gas accretion onto the discs of simulated Milky Way-mass galaxies
por: Iza, Federico, et al.
Publicado: (2023)