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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/235584
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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 Técnicas2025-09-29T09:42:44Zoai: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:34982025-09-29 09:42:44.745CONICET 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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13.070432 |