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SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust

hal.structure.identifierIstituto di Astrofisica e Planetologia Spaziali - INAF [IAPS]
dc.contributor.authorFERNÁNDEZ-ONTIVEROS, J. A.
dc.contributor.authorARMUS, L.
hal.structure.identifierUniversiteit Gent = Ghent University = Université de Gand [UGENT]
dc.contributor.authorBAES, M.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorBERNARD-SALAS, J.
dc.contributor.authorBOLATTO, A. D.
hal.structure.identifierFORMATION STELLAIRE 2017
dc.contributor.authorBRAINE, J.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorCIESLA, L.
hal.structure.identifierUniversiteit Gent = Ghent University = Université de Gand [UGENT]
dc.contributor.authorDE LOOZE, I.
hal.structure.identifierSteward Observatory
dc.contributor.authorEGAMI, E.
hal.structure.identifierFraunhofer Institute for Telecommunications - Heinrich Hertz Institute [Fraunhofer HHI]
dc.contributor.authorFISCHER, J.
hal.structure.identifierLaboratoire de Biométrie et Biologie Evolutive - UMR 5558 [LBBE]
dc.contributor.authorGIARD, M.
dc.contributor.authorGONZÁLEZ-ALFONSO, E.
hal.structure.identifierINAF - Osservatorio Astronomico di Padova [OAPD]
dc.contributor.authorGRANATO, G. L.
hal.structure.identifierINAF - Osservatorio Astronomico di Bologna [OABO]
dc.contributor.authorGRUPPIONI, C.
dc.contributor.authorIMANISHI, M.
dc.contributor.authorISHIHARA, D.
dc.contributor.authorKANEDA, H.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorMADDEN, S.
dc.contributor.authorMALKAN, M.
dc.contributor.authorMATSUHARA, H.
hal.structure.identifierUniversity of Manchester [Manchester]
dc.contributor.authorMATSUURA, M.
hal.structure.identifierResearch Center for Space and Cosmic Evolution [RCSCE]
dc.contributor.authorNAGAO, T.
dc.contributor.authorNAJARRO, F.
dc.contributor.authorNAKAGAWA, T.
dc.contributor.authorONAKA, T.
hal.structure.identifierDepartment of Environmental and Materials Engineering
dc.contributor.authorOYABU, S.
dc.contributor.authorPEREIRA-SANTAELLA, M.
dc.contributor.authorFOURNON, I. Pérez
dc.contributor.authorROELFSEMA, P.
hal.structure.identifierINAF - Osservatorio Astronomico di Roma [OAR]
dc.contributor.authorSANTINI, P.
hal.structure.identifierUniversidade Federal de Itajubá = Federal University of Itajubá
dc.contributor.authorSILVA, L.
dc.contributor.authorSMITH, J. -D. T.
hal.structure.identifierAntarctic Research a European Network for Astrophysics [ARENA]
dc.contributor.authorSPINOGLIO, L.
hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
dc.contributor.authorVAN DER TAK, F.
dc.contributor.authorWADA, T.
dc.contributor.authorWU, R.
dc.date.issued2017
dc.identifier.issn1323-3580
dc.description.abstractEnThe physical processes driving the chemical evolution of galaxies in the last $\sim 11\, \rm{Gyr}$ cannot be understood without directly probing the dust-obscured phase of star-forming galaxies and active galactic nuclei. This phase, hidden to optical tracers, represents the bulk of star formation and black hole accretion activity in galaxies at $1 < z < 3$. Spectroscopic observations with a cryogenic infrared (IR) observatory like SPICA will be sensitive enough to peer through the dust-obscured regions of galaxies and access the rest-frame mid- to far-IR range in galaxies at high-$z$. This wavelength range contains a unique suite of spectral lines and dust features that serve as proxies for the abundances of heavy elements and the dust composition, providing tracers with a feeble response to both extinction and temperature. In this work, we investigate how SPICA observations could be exploited to understand key aspects in the chemical evolution of galaxies: the assembly of nearby galaxies based on the spatial distribution of heavy element abundances, the global content of metals in galaxies reaching the knee of the luminosity function up to $z \sim 3$, and the dust composition of galaxies at high-$z$. Possible synergies with facilities available in the late 2020s are also discussed.
dc.language.isoen
dc.publisherCambridge University Press (CUP)
dc.title.enSPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
dc.typeArticle de revue
dc.identifier.doi10.1017/pasa.2017.43
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
dc.identifier.arxiv1710.02150
bordeaux.journalPublications of the Astronomical Society of Australia
bordeaux.pageid.e053
bordeaux.volume34
bordeaux.peerReviewedoui
hal.identifierhal-01613007
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01613007v1
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