Dust evolution with MUPPI in cosmological volumes

dc.creatorParente, Massimiliano
dc.creatorRagone Figueroa, Cinthia Judith
dc.creatorGranato, Gian Luigi
dc.creatorBorgani, Stefano
dc.creatorMurante, Giuseppe
dc.creatorValentini, Milena
dc.creatorBressan, Alessandro
dc.creatorLapi, Andrea
dc.date2022-09
dc.date.accessioned2023-08-30T23:53:23Z
dc.date.available2023-08-30T23:53:23Z
dc.identifierhttp://hdl.handle.net/11336/202771
dc.identifierParente, Massimiliano; Ragone Figueroa, Cinthia Judith; Granato, Gian Luigi; Borgani, Stefano; Murante, Giuseppe; et al.; Dust evolution with MUPPI in cosmological volumes; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 515; 2; 9-2022; 2053-2071
dc.identifier0035-8711
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8542878
dc.descriptionWe study the evolution of dust in a cosmological volume using a hydrodynamical simulation in which the dust production is coupled with the MUPPI (MUlti Phase Particle Integrator) sub-resolution model of star formation and feedback. As for the latter, we keep as reference the model setup calibrated previously to match the general properties of Milky Way-like galaxies in zoom-in simulations. However, we suggest that an increase of the star formation efficiency with the local dust-to-gas ratio would better reproduce the observed evolution of the cosmic star formation density. Moreover, the paucity of quenched galaxies at low redshift demands a stronger role of active galactic nucleus feedback. We tune the parameters ruling direct dust production from evolved stars and accretion in the interstellar medium to get scaling relations involving dust, stellar mass and metallicity in good agreement with observations. In low-mass galaxies, the accretion process is inefficient. As a consequence, they remain poorer in silicate and small grains than higher mass ones. We reproduce reasonably well the few available data on the radial distribution of dust outside the galactic region, supporting the assumption that the dust and gas dynamics are well coupled at galactic scales.
dc.descriptionFil: Parente, Massimiliano. Istituto Nazionale di Astrofisica; Italia. Scuola Internazionale Superiore Di Studi Avanzati; Italia
dc.descriptionFil: Ragone Figueroa, Cinthia Judith. 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
dc.descriptionFil: 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. Institute For Fundamental Physics Of The Universe; Italia. Istituto Nazionale di Astrofisica; Italia
dc.descriptionFil: Borgani, Stefano. Università degli Studi di Trieste; Italia. Institute For Fundamental Physics Of The Universe; Italia. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; Italia
dc.descriptionFil: Murante, Giuseppe. Istituto Nazionale di Astrofisica; Italia. Institute For Fundamental Physics Of The Universe; Italia
dc.descriptionFil: Valentini, Milena. Ludwig Maximilians Universitat; Alemania. Istituto Nazionale di Astrofisica; Italia. Excellence Cluster Origins; Italia
dc.descriptionFil: Bressan, Alessandro. Scuola Internazionale Superiore Di Studi Avanzati; Italia
dc.descriptionFil: Lapi, Andrea. Scuola Internazionale Superiore Di Studi Avanzati; Italia. Istituto Di Radioastronomia; Italia. Institute For Fundamental Physics Of The Universe; Italia. Istituto Nazionale di Fisica Nucleare; Italia
dc.formatapplication/pdf
dc.formatapplication/pdf
dc.languageeng
dc.publisherOxford University Press
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac1913
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/515/2/2053/6646521?redirectedFrom=fulltext
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subjectDUST, EXTINCTION
dc.subjectGALAXIES: EVOLUTION
dc.subjectGALAXIES: FORMATION
dc.subjectGALAXIES: GENERAL
dc.subjectGALAXIES: ISM
dc.subjectMETHODS: NUMERICAL
dc.subjecthttps://purl.org/becyt/ford/1.3
dc.subjecthttps://purl.org/becyt/ford/1
dc.titleDust evolution with MUPPI in cosmological volumes
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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