The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework

Autores
Parente, Massimiliano; Ragone Figueroa, Cinthia Judith; Granato, Gian Luigi; Lapi, Andrea
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Observations suggest that the amount of galactic dust in the Universe decreased by a factor of ∼2–3 during the last ∼8 Gyr. However, cosmological models of galaxy evolution usually struggle to explain this decrease. Here, we use the semi-analytic model (SAM) L-GALAXIES2020 to show that this drop may be reproduced assuming standard prescriptions for dust productionand evolution. We extend the SAM with (i) a state-of-the-art dust model that adopts the two-size approximation and (ii) a new disc instability criterion that triggers bulge and central black hole growth. The model reproduces some fundamental properties of the local galaxy population, such as the fraction of spheroid-dominated galaxies and some scaling relations involving dust.Moreover, the model predicts a galactic dust drop from z ∼ 1 → 0, which becomes closer to the observed one when adopting the new treatment of disc instabilities. This result is related to the newly implemented supermassive black hole growth during disc instabilities, which enhances the quenching of massive galaxies. Consequently, these objects feature a lower gas and dust content.We provide a census of the contribution of all the processes affecting the galactic dust content. Accretion is the dominant dust mass growth process. Destruction by supernovae, astration and ejection by winds have all a non-negligible role in decreasing the overall dust content in galaxies below z ∼ 1. We also discuss predictions concerning extra-galactic dust, confirming that asputtering efficiency lower than the canonical one is required to match the few available observations.
Fil: Parente, Massimiliano. Scuola Internazionale Superiore Di Studi Avanzati (sissa);
Fil: Ragone Figueroa, Cinthia Judith. Istituto Nazionale di Astrofisica; Italia. 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: Granato, Gian Luigi. 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. Istituto Nazionale di Astrofisica; Italia
Fil: Lapi, Andrea. Scuola Internazionale Superiore Di Studi Avanzati (sissa); . Istituto Nazionale di Astrofisica; Italia
Materia
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: GENERAL
GALAXIES: ISM
DUST, EXTINTION
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:11336/235584
Acceder
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network_name_str CONICET Digital (CONICET)
spelling The z ≲ 1 drop of cosmic dust abundance in a semi-analytic frameworkParente, MassimilianoRagone Figueroa, Cinthia JudithGranato, Gian LuigiLapi, AndreaGALAXIES: EVOLUTIONGALAXIES: FORMATIONGALAXIES: GENERALGALAXIES: ISMDUST, EXTINTIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Observations suggest that the amount of galactic dust in the Universe decreased by a factor of ∼2–3 during the last ∼8 Gyr. However, cosmological models of galaxy evolution usually struggle to explain this decrease. Here, we use the semi-analytic model (SAM) L-GALAXIES2020 to show that this drop may be reproduced assuming standard prescriptions for dust productionand evolution. We extend the SAM with (i) a state-of-the-art dust model that adopts the two-size approximation and (ii) a new disc instability criterion that triggers bulge and central black hole growth. The model reproduces some fundamental properties of the local galaxy population, such as the fraction of spheroid-dominated galaxies and some scaling relations involving dust.Moreover, the model predicts a galactic dust drop from z ∼ 1 → 0, which becomes closer to the observed one when adopting the new treatment of disc instabilities. This result is related to the newly implemented supermassive black hole growth during disc instabilities, which enhances the quenching of massive galaxies. Consequently, these objects feature a lower gas and dust content.We provide a census of the contribution of all the processes affecting the galactic dust content. Accretion is the dominant dust mass growth process. Destruction by supernovae, astration and ejection by winds have all a non-negligible role in decreasing the overall dust content in galaxies below z ∼ 1. We also discuss predictions concerning extra-galactic dust, confirming that asputtering efficiency lower than the canonical one is required to match the few available observations.Fil: Parente, Massimiliano. Scuola Internazionale Superiore Di Studi Avanzati (sissa);Fil: Ragone Figueroa, Cinthia Judith. Istituto Nazionale di Astrofisica; Italia. 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: Granato, Gian Luigi. 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. Istituto Nazionale di Astrofisica; ItaliaFil: Lapi, Andrea. Scuola Internazionale Superiore Di Studi Avanzati (sissa); . Istituto Nazionale di Astrofisica; ItaliaOxford University Press2023-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/235584Parente, Massimiliano; Ragone Figueroa, Cinthia Judith; Granato, Gian Luigi; Lapi, Andrea; The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 521; 4; 3-2023; 6105-61231365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad907info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:11:20Zoai:ri.conicet.gov.ar:11336/235584instacron: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:34982025-10-22 11:11:20.666CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
title The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
spellingShingle The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
Parente, Massimiliano
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: GENERAL
GALAXIES: ISM
DUST, EXTINTION
title_short The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
title_full The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
title_fullStr The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
title_full_unstemmed The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
title_sort The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework
dc.creator.none.fl_str_mv Parente, Massimiliano
Ragone Figueroa, Cinthia Judith
Granato, Gian Luigi
Lapi, Andrea
author Parente, Massimiliano
author_facet Parente, Massimiliano
Ragone Figueroa, Cinthia Judith
Granato, Gian Luigi
Lapi, Andrea
author_role author
author2 Ragone Figueroa, Cinthia Judith
Granato, Gian Luigi
Lapi, Andrea
author2_role author
author
author
dc.subject.none.fl_str_mv GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: GENERAL
GALAXIES: ISM
DUST, EXTINTION
topic GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: GENERAL
GALAXIES: ISM
DUST, EXTINTION
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Observations suggest that the amount of galactic dust in the Universe decreased by a factor of ∼2–3 during the last ∼8 Gyr. However, cosmological models of galaxy evolution usually struggle to explain this decrease. Here, we use the semi-analytic model (SAM) L-GALAXIES2020 to show that this drop may be reproduced assuming standard prescriptions for dust productionand evolution. We extend the SAM with (i) a state-of-the-art dust model that adopts the two-size approximation and (ii) a new disc instability criterion that triggers bulge and central black hole growth. The model reproduces some fundamental properties of the local galaxy population, such as the fraction of spheroid-dominated galaxies and some scaling relations involving dust.Moreover, the model predicts a galactic dust drop from z ∼ 1 → 0, which becomes closer to the observed one when adopting the new treatment of disc instabilities. This result is related to the newly implemented supermassive black hole growth during disc instabilities, which enhances the quenching of massive galaxies. Consequently, these objects feature a lower gas and dust content.We provide a census of the contribution of all the processes affecting the galactic dust content. Accretion is the dominant dust mass growth process. Destruction by supernovae, astration and ejection by winds have all a non-negligible role in decreasing the overall dust content in galaxies below z ∼ 1. We also discuss predictions concerning extra-galactic dust, confirming that asputtering efficiency lower than the canonical one is required to match the few available observations.
Fil: Parente, Massimiliano. Scuola Internazionale Superiore Di Studi Avanzati (sissa);
Fil: Ragone Figueroa, Cinthia Judith. Istituto Nazionale di Astrofisica; Italia. 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: Granato, Gian Luigi. 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. Istituto Nazionale di Astrofisica; Italia
Fil: Lapi, Andrea. Scuola Internazionale Superiore Di Studi Avanzati (sissa); . Istituto Nazionale di Astrofisica; Italia
description Observations suggest that the amount of galactic dust in the Universe decreased by a factor of ∼2–3 during the last ∼8 Gyr. However, cosmological models of galaxy evolution usually struggle to explain this decrease. Here, we use the semi-analytic model (SAM) L-GALAXIES2020 to show that this drop may be reproduced assuming standard prescriptions for dust productionand evolution. We extend the SAM with (i) a state-of-the-art dust model that adopts the two-size approximation and (ii) a new disc instability criterion that triggers bulge and central black hole growth. The model reproduces some fundamental properties of the local galaxy population, such as the fraction of spheroid-dominated galaxies and some scaling relations involving dust.Moreover, the model predicts a galactic dust drop from z ∼ 1 → 0, which becomes closer to the observed one when adopting the new treatment of disc instabilities. This result is related to the newly implemented supermassive black hole growth during disc instabilities, which enhances the quenching of massive galaxies. Consequently, these objects feature a lower gas and dust content.We provide a census of the contribution of all the processes affecting the galactic dust content. Accretion is the dominant dust mass growth process. Destruction by supernovae, astration and ejection by winds have all a non-negligible role in decreasing the overall dust content in galaxies below z ∼ 1. We also discuss predictions concerning extra-galactic dust, confirming that asputtering efficiency lower than the canonical one is required to match the few available observations.
publishDate 2023
dc.date.none.fl_str_mv 2023-03
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/11336/235584
Parente, Massimiliano; Ragone Figueroa, Cinthia Judith; Granato, Gian Luigi; Lapi, Andrea; The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 521; 4; 3-2023; 6105-6123
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/235584
identifier_str_mv Parente, Massimiliano; Ragone Figueroa, Cinthia Judith; Granato, Gian Luigi; Lapi, Andrea; The z ≲ 1 drop of cosmic dust abundance in a semi-analytic framework; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 521; 4; 3-2023; 6105-6123
1365-2966
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad907
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 Oxford University Press
publisher.none.fl_str_mv Oxford University Press
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 12.982451

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