Local metallicity in simulated galaxies

In the last decade, integral field spectroscopy has expanded our understanding of chemical evolution of galaxies, giving evidence of a radial gradient of gas-phase metallicity. In this work, we use the state-of-art hydrodynamical simulation EAGLE to study the resolved, local properties of galaxies....

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Autores principales: Collacchioni, Florencia, Correa, Camila Anahí, Lagos, C. D. P., Cora, Sofía Alejandra
Formato: Articulo
Lenguaje:Inglés
Publicado: 2021
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/171020
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spelling I19-R120-10915-1710202024-10-02T20:04:30Z http://sedici.unlp.edu.ar/handle/10915/171020 Local metallicity in simulated galaxies Collacchioni, Florencia Correa, Camila Anahí Lagos, C. D. P. Cora, Sofía Alejandra 2021 2024-10-02T13:51:20Z en Ciencias Astronómicas methods: numerical galaxies: evolution galaxies: formation In the last decade, integral field spectroscopy has expanded our understanding of chemical evolution of galaxies, giving evidence of a radial gradient of gas-phase metallicity. In this work, we use the state-of-art hydrodynamical simulation EAGLE to study the resolved, local properties of galaxies. We show that the local gas metallicity correlates with the stellar mass surface density and anti-correlates with the gas accretion. Resolved metallicity profiles acts as a good estimator of gas accretion, and can be used to understand the changes in the chemical enrichment of galaxies. En la última década, la espectroscopia de campo integrado ha expandido nuestra comprensión de la evolución química de las galaxias, dando evidencia de un gradiente radial de la metalicidad de la fase gaseosa. En este trabajo, usamos la simulación cosmológica hidrodinámica EAGLE para estudiar las propiedades localmente resueltas de las galaxias. Mostramos que la metalicidad local del gas correlaciona con la densidad superficial de masa estelar y anticorrelaciona con la acreción de gas. Los perfiles de metalicidad resueltos actúan como buenos estimadores de la acreción de gas, y pueden ser usados para entender los cambios en el enriquecimiento químico de las galaxias. Asociación Argentina de Astronomía Articulo Articulo http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 165-167
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
methods: numerical
galaxies: evolution
galaxies: formation
spellingShingle Ciencias Astronómicas
methods: numerical
galaxies: evolution
galaxies: formation
Collacchioni, Florencia
Correa, Camila Anahí
Lagos, C. D. P.
Cora, Sofía Alejandra
Local metallicity in simulated galaxies
topic_facet Ciencias Astronómicas
methods: numerical
galaxies: evolution
galaxies: formation
description In the last decade, integral field spectroscopy has expanded our understanding of chemical evolution of galaxies, giving evidence of a radial gradient of gas-phase metallicity. In this work, we use the state-of-art hydrodynamical simulation EAGLE to study the resolved, local properties of galaxies. We show that the local gas metallicity correlates with the stellar mass surface density and anti-correlates with the gas accretion. Resolved metallicity profiles acts as a good estimator of gas accretion, and can be used to understand the changes in the chemical enrichment of galaxies.
format Articulo
Articulo
author Collacchioni, Florencia
Correa, Camila Anahí
Lagos, C. D. P.
Cora, Sofía Alejandra
author_facet Collacchioni, Florencia
Correa, Camila Anahí
Lagos, C. D. P.
Cora, Sofía Alejandra
author_sort Collacchioni, Florencia
title Local metallicity in simulated galaxies
title_short Local metallicity in simulated galaxies
title_full Local metallicity in simulated galaxies
title_fullStr Local metallicity in simulated galaxies
title_full_unstemmed Local metallicity in simulated galaxies
title_sort local metallicity in simulated galaxies
publishDate 2021
url http://sedici.unlp.edu.ar/handle/10915/171020
work_keys_str_mv AT collacchioniflorencia localmetallicityinsimulatedgalaxies
AT correacamilaanahi localmetallicityinsimulatedgalaxies
AT lagoscdp localmetallicityinsimulatedgalaxies
AT corasofiaalejandra localmetallicityinsimulatedgalaxies
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