Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations

Autores
Zerbo, María Candela; de Rossi, Maria Emilia; Lara López, M. A.; Cora, Sofia Alejandra; Zenocratti, Lucas Jesús
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Effective yields, eff, are defined by fundamental galaxy properties (i.e., stellar mass -★-, gas mass -gas- and gas-phase metallicity). For a closed-box model, eff is constant and equivalent to the mass in metals returned to the gas per unit mass locked in long-lived stars. Deviations from such behaviour have been often considered observational signatures of past feedback events. By analysing EAGLE simulations with different feedback models, we evaluate the impact of supernovae (SN) and active galactic nuclei (AGN) feedback on eff at redshift = 0. When removing supermassive black holes (BH) and, hence, AGN effects, in simulations, galaxies are located around a plane in the ★ − gas − O/H parameter space (being O/H a proxy for gas metallicity, as usual), with such a plane roughly describing a surface of constant eff. As the ratio between BH mass and ★ increases, galaxies deviate from that plane towards lower eff as a consequence of AGN feedback. For galaxies not strongly affected by AGN feedback, a stronger SN feedback efficiency generates deviations towards lower eff, while galaxies move towards the opposite side of the plane (i.e., towards higher values of eff) as SN feedback becomes weaker. Star-forming galaxies observed in the Local Universe are located around a similar 3D plane. Our results suggest that the features of the scatter around the observed plane are related to the different feedback histories of galaxies, which might be traced by eff.
Fil: Zerbo, María Candela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: de Rossi, Maria Emilia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Lara López, M. A.. Universidad Complutense de Madrid; España
Fil: Cora, Sofia Alejandra. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Zenocratti, Lucas Jesús. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Materia
GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: FUNDAMENTAL PARAMETERS
GALAXIES: STAR FORMATION
METHODS: NUMERICAL
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/233034
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/233034
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulationsZerbo, María Candelade Rossi, Maria EmiliaLara López, M. A.Cora, Sofia AlejandraZenocratti, Lucas JesúsGALAXIES: ABUNDANCESGALAXIES: EVOLUTIONGALAXIES: FORMATIONGALAXIES: FUNDAMENTAL PARAMETERSGALAXIES: STAR FORMATIONMETHODS: NUMERICALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Effective yields, eff, are defined by fundamental galaxy properties (i.e., stellar mass -★-, gas mass -gas- and gas-phase metallicity). For a closed-box model, eff is constant and equivalent to the mass in metals returned to the gas per unit mass locked in long-lived stars. Deviations from such behaviour have been often considered observational signatures of past feedback events. By analysing EAGLE simulations with different feedback models, we evaluate the impact of supernovae (SN) and active galactic nuclei (AGN) feedback on eff at redshift = 0. When removing supermassive black holes (BH) and, hence, AGN effects, in simulations, galaxies are located around a plane in the ★ − gas − O/H parameter space (being O/H a proxy for gas metallicity, as usual), with such a plane roughly describing a surface of constant eff. As the ratio between BH mass and ★ increases, galaxies deviate from that plane towards lower eff as a consequence of AGN feedback. For galaxies not strongly affected by AGN feedback, a stronger SN feedback efficiency generates deviations towards lower eff, while galaxies move towards the opposite side of the plane (i.e., towards higher values of eff) as SN feedback becomes weaker. Star-forming galaxies observed in the Local Universe are located around a similar 3D plane. Our results suggest that the features of the scatter around the observed plane are related to the different feedback histories of galaxies, which might be traced by eff.Fil: Zerbo, María Candela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: de Rossi, Maria Emilia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Lara López, M. A.. Universidad Complutense de Madrid; EspañaFil: Cora, Sofia Alejandra. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Zenocratti, Lucas Jesús. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaWiley Blackwell Publishing, Inc2024-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/233034Zerbo, María Candela; de Rossi, Maria Emilia; Lara López, M. A.; Cora, Sofia Alejandra; Zenocratti, Lucas Jesús; Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 2-2024; 1-200035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stae490/7609701info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae490info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:40:10Zoai:ri.conicet.gov.ar:11336/233034instacron: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:34982025-10-15 15:40:11.197CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
title Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
spellingShingle Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
Zerbo, María Candela
GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: FUNDAMENTAL PARAMETERS
GALAXIES: STAR FORMATION
METHODS: NUMERICAL
title_short Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
title_full Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
title_fullStr Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
title_full_unstemmed Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
title_sort Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
dc.creator.none.fl_str_mv Zerbo, María Candela
de Rossi, Maria Emilia
Lara López, M. A.
Cora, Sofia Alejandra
Zenocratti, Lucas Jesús
author Zerbo, María Candela
author_facet Zerbo, María Candela
de Rossi, Maria Emilia
Lara López, M. A.
Cora, Sofia Alejandra
Zenocratti, Lucas Jesús
author_role author
author2 de Rossi, Maria Emilia
Lara López, M. A.
Cora, Sofia Alejandra
Zenocratti, Lucas Jesús
author2_role author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: FUNDAMENTAL PARAMETERS
GALAXIES: STAR FORMATION
METHODS: NUMERICAL
topic GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: FUNDAMENTAL PARAMETERS
GALAXIES: STAR FORMATION
METHODS: NUMERICAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Effective yields, eff, are defined by fundamental galaxy properties (i.e., stellar mass -★-, gas mass -gas- and gas-phase metallicity). For a closed-box model, eff is constant and equivalent to the mass in metals returned to the gas per unit mass locked in long-lived stars. Deviations from such behaviour have been often considered observational signatures of past feedback events. By analysing EAGLE simulations with different feedback models, we evaluate the impact of supernovae (SN) and active galactic nuclei (AGN) feedback on eff at redshift = 0. When removing supermassive black holes (BH) and, hence, AGN effects, in simulations, galaxies are located around a plane in the ★ − gas − O/H parameter space (being O/H a proxy for gas metallicity, as usual), with such a plane roughly describing a surface of constant eff. As the ratio between BH mass and ★ increases, galaxies deviate from that plane towards lower eff as a consequence of AGN feedback. For galaxies not strongly affected by AGN feedback, a stronger SN feedback efficiency generates deviations towards lower eff, while galaxies move towards the opposite side of the plane (i.e., towards higher values of eff) as SN feedback becomes weaker. Star-forming galaxies observed in the Local Universe are located around a similar 3D plane. Our results suggest that the features of the scatter around the observed plane are related to the different feedback histories of galaxies, which might be traced by eff.
Fil: Zerbo, María Candela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: de Rossi, Maria Emilia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Lara López, M. A.. Universidad Complutense de Madrid; España
Fil: Cora, Sofia Alejandra. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Zenocratti, Lucas Jesús. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
description Effective yields, eff, are defined by fundamental galaxy properties (i.e., stellar mass -★-, gas mass -gas- and gas-phase metallicity). For a closed-box model, eff is constant and equivalent to the mass in metals returned to the gas per unit mass locked in long-lived stars. Deviations from such behaviour have been often considered observational signatures of past feedback events. By analysing EAGLE simulations with different feedback models, we evaluate the impact of supernovae (SN) and active galactic nuclei (AGN) feedback on eff at redshift = 0. When removing supermassive black holes (BH) and, hence, AGN effects, in simulations, galaxies are located around a plane in the ★ − gas − O/H parameter space (being O/H a proxy for gas metallicity, as usual), with such a plane roughly describing a surface of constant eff. As the ratio between BH mass and ★ increases, galaxies deviate from that plane towards lower eff as a consequence of AGN feedback. For galaxies not strongly affected by AGN feedback, a stronger SN feedback efficiency generates deviations towards lower eff, while galaxies move towards the opposite side of the plane (i.e., towards higher values of eff) as SN feedback becomes weaker. Star-forming galaxies observed in the Local Universe are located around a similar 3D plane. Our results suggest that the features of the scatter around the observed plane are related to the different feedback histories of galaxies, which might be traced by eff.
publishDate 2024
dc.date.none.fl_str_mv 2024-02
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/11336/233034
Zerbo, María Candela; de Rossi, Maria Emilia; Lara López, M. A.; Cora, Sofia Alejandra; Zenocratti, Lucas Jesús; Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 2-2024; 1-20
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/233034
identifier_str_mv Zerbo, María Candela; de Rossi, Maria Emilia; Lara López, M. A.; Cora, Sofia Alejandra; Zenocratti, Lucas Jesús; Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 2-2024; 1-20
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/advance-article/doi/10.1093/mnras/stae490/7609701
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae490
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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score 13.22299

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