The evolution of the metallicity gradient and the star formation efficiency in disc galaxies
- Autores
- Sillero Ros, Guillermo Emanuel; Tissera, Patricia Beatriz; Garcia Lambas, Diego Rodolfo; Michel-Dansac, Leopold Laurent Joseph
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We study the oxygen abundance profiles of the gas-phase components in hydrodynamical simulations of pre-prepared disc galaxies including major mergers, close encounters and isolated configurations. We analyse the evolution of the slope of oxygen abundance profiles and the specific star formation rate (sSFR) along their evolution. We find that galaxy-galaxy interactions could generate either positive or negative gas-phase oxygen profiles, depending on the state of evolution. Along the interaction, galaxies are found to have metallicity gradients and sSFR consistent with observations, on average. Strong gas inflows produced during galaxy- galaxy interactions or as a result of strong local instabilities in gas-rich discs are able to produce both a quick dilution of the central gas-phase metallicity and a sudden increase of the sSFR. Our simulations show that, during these events, a correlation between the metallicity gradients and the sSFR can be set up if strong gas inflows are triggered in the central regions in short time-scales. Simulated galaxies without experiencing strong disturbances evolve smoothly without modifying the metallicity gradients. Gas-rich systems show large dispersion along the correlation. The dispersion in the observed relation could be interpreted as produced by the combination of galaxies with different gas-richness and/or experiencing different types of interactions. Hence, our findings suggest that the observed relation might be the smoking gun of galaxies forming in a hierarchical clustering scenario.
Fil: Sillero Ros, Guillermo Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Tissera, Patricia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Andrés Bello; Chile
Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Michel-Dansac, Leopold Laurent Joseph. Centre de Recherche Astrophysique de Lyon; Francia. Université Claude Bernard Lyon 1; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina - Materia
-
DARK MATTER
GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/64869
Ver los metadatos del registro completo
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The evolution of the metallicity gradient and the star formation efficiency in disc galaxiesSillero Ros, Guillermo EmanuelTissera, Patricia BeatrizGarcia Lambas, Diego RodolfoMichel-Dansac, Leopold Laurent JosephDARK MATTERGALAXIES: ABUNDANCESGALAXIES: EVOLUTIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the oxygen abundance profiles of the gas-phase components in hydrodynamical simulations of pre-prepared disc galaxies including major mergers, close encounters and isolated configurations. We analyse the evolution of the slope of oxygen abundance profiles and the specific star formation rate (sSFR) along their evolution. We find that galaxy-galaxy interactions could generate either positive or negative gas-phase oxygen profiles, depending on the state of evolution. Along the interaction, galaxies are found to have metallicity gradients and sSFR consistent with observations, on average. Strong gas inflows produced during galaxy- galaxy interactions or as a result of strong local instabilities in gas-rich discs are able to produce both a quick dilution of the central gas-phase metallicity and a sudden increase of the sSFR. Our simulations show that, during these events, a correlation between the metallicity gradients and the sSFR can be set up if strong gas inflows are triggered in the central regions in short time-scales. Simulated galaxies without experiencing strong disturbances evolve smoothly without modifying the metallicity gradients. Gas-rich systems show large dispersion along the correlation. The dispersion in the observed relation could be interpreted as produced by the combination of galaxies with different gas-richness and/or experiencing different types of interactions. Hence, our findings suggest that the observed relation might be the smoking gun of galaxies forming in a hierarchical clustering scenario.Fil: Sillero Ros, Guillermo Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Tissera, Patricia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Andrés Bello; ChileFil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Michel-Dansac, Leopold Laurent Joseph. Centre de Recherche Astrophysique de Lyon; Francia. Université Claude Bernard Lyon 1; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaWiley Blackwell Publishing, Inc2017-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/64869Sillero Ros, Guillermo Emanuel; Tissera, Patricia Beatriz; Garcia Lambas, Diego Rodolfo; Michel-Dansac, Leopold Laurent Joseph; The evolution of the metallicity gradient and the star formation efficiency in disc galaxies; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 472; 4; 12-2017; 4404-44130035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/472/4/4404/4103564info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx2265info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:52:31Zoai:ri.conicet.gov.ar:11336/64869instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:52:31.954CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
title |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
spellingShingle |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies Sillero Ros, Guillermo Emanuel DARK MATTER GALAXIES: ABUNDANCES GALAXIES: EVOLUTION |
title_short |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
title_full |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
title_fullStr |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
title_full_unstemmed |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
title_sort |
The evolution of the metallicity gradient and the star formation efficiency in disc galaxies |
dc.creator.none.fl_str_mv |
Sillero Ros, Guillermo Emanuel Tissera, Patricia Beatriz Garcia Lambas, Diego Rodolfo Michel-Dansac, Leopold Laurent Joseph |
author |
Sillero Ros, Guillermo Emanuel |
author_facet |
Sillero Ros, Guillermo Emanuel Tissera, Patricia Beatriz Garcia Lambas, Diego Rodolfo Michel-Dansac, Leopold Laurent Joseph |
author_role |
author |
author2 |
Tissera, Patricia Beatriz Garcia Lambas, Diego Rodolfo Michel-Dansac, Leopold Laurent Joseph |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
DARK MATTER GALAXIES: ABUNDANCES GALAXIES: EVOLUTION |
topic |
DARK MATTER GALAXIES: ABUNDANCES GALAXIES: EVOLUTION |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We study the oxygen abundance profiles of the gas-phase components in hydrodynamical simulations of pre-prepared disc galaxies including major mergers, close encounters and isolated configurations. We analyse the evolution of the slope of oxygen abundance profiles and the specific star formation rate (sSFR) along their evolution. We find that galaxy-galaxy interactions could generate either positive or negative gas-phase oxygen profiles, depending on the state of evolution. Along the interaction, galaxies are found to have metallicity gradients and sSFR consistent with observations, on average. Strong gas inflows produced during galaxy- galaxy interactions or as a result of strong local instabilities in gas-rich discs are able to produce both a quick dilution of the central gas-phase metallicity and a sudden increase of the sSFR. Our simulations show that, during these events, a correlation between the metallicity gradients and the sSFR can be set up if strong gas inflows are triggered in the central regions in short time-scales. Simulated galaxies without experiencing strong disturbances evolve smoothly without modifying the metallicity gradients. Gas-rich systems show large dispersion along the correlation. The dispersion in the observed relation could be interpreted as produced by the combination of galaxies with different gas-richness and/or experiencing different types of interactions. Hence, our findings suggest that the observed relation might be the smoking gun of galaxies forming in a hierarchical clustering scenario. Fil: Sillero Ros, Guillermo Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Tissera, Patricia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Andrés Bello; Chile Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Michel-Dansac, Leopold Laurent Joseph. Centre de Recherche Astrophysique de Lyon; Francia. Université Claude Bernard Lyon 1; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina |
description |
We study the oxygen abundance profiles of the gas-phase components in hydrodynamical simulations of pre-prepared disc galaxies including major mergers, close encounters and isolated configurations. We analyse the evolution of the slope of oxygen abundance profiles and the specific star formation rate (sSFR) along their evolution. We find that galaxy-galaxy interactions could generate either positive or negative gas-phase oxygen profiles, depending on the state of evolution. Along the interaction, galaxies are found to have metallicity gradients and sSFR consistent with observations, on average. Strong gas inflows produced during galaxy- galaxy interactions or as a result of strong local instabilities in gas-rich discs are able to produce both a quick dilution of the central gas-phase metallicity and a sudden increase of the sSFR. Our simulations show that, during these events, a correlation between the metallicity gradients and the sSFR can be set up if strong gas inflows are triggered in the central regions in short time-scales. Simulated galaxies without experiencing strong disturbances evolve smoothly without modifying the metallicity gradients. Gas-rich systems show large dispersion along the correlation. The dispersion in the observed relation could be interpreted as produced by the combination of galaxies with different gas-richness and/or experiencing different types of interactions. Hence, our findings suggest that the observed relation might be the smoking gun of galaxies forming in a hierarchical clustering scenario. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/64869 Sillero Ros, Guillermo Emanuel; Tissera, Patricia Beatriz; Garcia Lambas, Diego Rodolfo; Michel-Dansac, Leopold Laurent Joseph; The evolution of the metallicity gradient and the star formation efficiency in disc galaxies; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 472; 4; 12-2017; 4404-4413 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/64869 |
identifier_str_mv |
Sillero Ros, Guillermo Emanuel; Tissera, Patricia Beatriz; Garcia Lambas, Diego Rodolfo; Michel-Dansac, Leopold Laurent Joseph; The evolution of the metallicity gradient and the star formation efficiency in disc galaxies; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 472; 4; 12-2017; 4404-4413 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/472/4/4404/4103564 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx2265 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613610934894592 |
score |
13.070432 |