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Probing the baryon cycle of galaxies with SPICA mid- and far-infrared observations

hal.structure.identifierKapteyn Astronomical Institute [Groningen]
dc.contributor.authorVAN DER TAK, F. F. S.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorMADDEN, S. C.
dc.contributor.authorROELFSEMA, P.
dc.contributor.authorARMUS, L.
hal.structure.identifierSterrenkundig Observatorium
dc.contributor.authorBAES, M.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorBERNARD-SALAS, J.
hal.structure.identifierDepartment of Astronomy [College Park]
dc.contributor.authorBOLATTO, A.
hal.structure.identifierFORMATION STELLAIRE 2018
dc.contributor.authorBONTEMPS, Sylvain
hal.structure.identifierObservatoire astronomique de Strasbourg [OAS]
dc.contributor.authorBOT, C.
dc.contributor.authorBRADFORD, C. M.
hal.structure.identifierFORMATION STELLAIRE 2018
dc.contributor.authorBRAINE, J.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorCIESLA, L.
dc.contributor.authorCLEMENTS, D.
hal.structure.identifierZentrum für Astronomie der Universität Heidelberg [ZAH]
dc.contributor.authorCORMIER, D.
hal.structure.identifierIstituto di Astrofisica e Planetologia Spaziali - INAF [IAPS]
dc.contributor.authorFERNÁNDEZ-ONTIVEROS, J. A.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorGALLIANO, F.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorGIARD, M.
hal.structure.identifierUniversity of Zaragoza - Universidad de Zaragoza [Zaragoza]
dc.contributor.authorGÓMEZ, H.
dc.contributor.authorGONZÁLEZ-ALFONSO, E.
hal.structure.identifierFormation Stellaire
dc.contributor.authorHERPIN, Fabrice
hal.structure.identifierNatl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7 Canada
dc.contributor.authorJOHNSTONE, D.
dc.contributor.authorJONES, A.
dc.contributor.authorKANEDA, H.
dc.contributor.authorKEMPER, F.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorLEBOUTEILLER, V.
hal.structure.identifierSterrenkundig Observatorium
dc.contributor.authorDE LOOZE, I.
hal.structure.identifierUniversity of Manchester [Manchester]
dc.contributor.authorMATSUURA, M.
dc.contributor.authorNAKAGAWA, T.
dc.contributor.authorONAKA, T.
dc.contributor.authorPÉREZ-GONZÁLEZ, P.
hal.structure.identifierforeign laboratories [FL]
dc.contributor.authorSHIPMAN, R.
hal.structure.identifierAntarctic Research a European Network for Astrophysics [ARENA]
dc.contributor.authorSPINOGLIO, L.
dc.date.issued2018
dc.identifier.issn1323-3580
dc.description.abstractEnThe SPICA mid and far-infrared telescope will address fundamental issues in our understanding of star formation and ISM physics in galaxies. A particular hallmark of SPICA is the outstanding sensitivity enabled by the cold telescope, optimized detectors, and wide instantaneous bandwidth throughout the mid- and far-infrared. The spectroscopic, imaging and polarimetric observations that SPICA will be able to collect will help in clarifying the complex physical mechanisms which underlie the baryon cycle of galaxies. In particular: (i) The access to a large suite of atomic and ionic fine-structure lines for large samples of galaxies will shed light on the origin of the observed spread in star formation rates within and between galaxies. (ii) Observations of HD rotational lines (out to $\sim$10 Mpc) and fine structure lines such as [CII] 158 $\mu$m (out to $\sim$100 Mpc) will clarify the main reservoirs of interstellar matter in galaxies, including phases where CO does not emit. (iii) Far-infrared spectroscopy of dust and ice features will address uncertainties in the mass and composition of dust in galaxies, and the contributions of supernovae to the interstellar dust budget will be quantified by photometry and monitoring of supernova remnants in nearby galaxies. (iv) Observations of far-infrared cooling lines such as [OI] 63 $\mu$m from star-forming molecular clouds in our Galaxy will evaluate the importance of shocks to dissipate turbulent energy. The paper concludes with requirements for the telescope and instruments, and recommendations for the observing strategy.
dc.language.isoen
dc.publisherCambridge University Press (CUP)
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enProbing the baryon cycle of galaxies with SPICA mid- and far-infrared observations
dc.typeArticle de revue
dc.identifier.doi10.1017/pasa.2017.67
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
dc.identifier.arxiv1711.11327
bordeaux.journalPublications of the Astronomical Society of Australia
bordeaux.pageid.e002
bordeaux.volume35
bordeaux.peerReviewedoui
hal.identifierhal-01655546
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01655546v1
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