Probing the baryon cycle of galaxies with SPICA mid- and far-infrared observations
hal.structure.identifier | Kapteyn Astronomical Institute [Groningen] | |
dc.contributor.author | VAN DER TAK, F. F. S. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | MADDEN, S. C. | |
dc.contributor.author | ROELFSEMA, P. | |
dc.contributor.author | ARMUS, L. | |
hal.structure.identifier | Sterrenkundig Observatorium | |
dc.contributor.author | BAES, M. | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | BERNARD-SALAS, J. | |
hal.structure.identifier | Department of Astronomy [College Park] | |
dc.contributor.author | BOLATTO, A. | |
hal.structure.identifier | FORMATION STELLAIRE 2018 | |
dc.contributor.author | BONTEMPS, Sylvain | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [OAS] | |
dc.contributor.author | BOT, C. | |
dc.contributor.author | BRADFORD, C. M. | |
hal.structure.identifier | FORMATION STELLAIRE 2018 | |
dc.contributor.author | BRAINE, J. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | CIESLA, L. | |
dc.contributor.author | CLEMENTS, D. | |
hal.structure.identifier | Zentrum für Astronomie der Universität Heidelberg [ZAH] | |
dc.contributor.author | CORMIER, D. | |
hal.structure.identifier | Istituto di Astrofisica e Planetologia Spaziali - INAF [IAPS] | |
dc.contributor.author | FERNÁNDEZ-ONTIVEROS, J. A. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | GALLIANO, F. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | GIARD, M. | |
hal.structure.identifier | University of Zaragoza - Universidad de Zaragoza [Zaragoza] | |
dc.contributor.author | GÓMEZ, H. | |
dc.contributor.author | GONZÁLEZ-ALFONSO, E. | |
hal.structure.identifier | Formation Stellaire | |
dc.contributor.author | HERPIN, Fabrice | |
hal.structure.identifier | Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7 Canada | |
dc.contributor.author | JOHNSTONE, D. | |
dc.contributor.author | JONES, A. | |
dc.contributor.author | KANEDA, H. | |
dc.contributor.author | KEMPER, F. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | LEBOUTEILLER, V. | |
hal.structure.identifier | Sterrenkundig Observatorium | |
dc.contributor.author | DE LOOZE, I. | |
hal.structure.identifier | University of Manchester [Manchester] | |
dc.contributor.author | MATSUURA, M. | |
dc.contributor.author | NAKAGAWA, T. | |
dc.contributor.author | ONAKA, T. | |
dc.contributor.author | PÉREZ-GONZÁLEZ, P. | |
hal.structure.identifier | foreign laboratories [FL] | |
dc.contributor.author | SHIPMAN, R. | |
hal.structure.identifier | Antarctic Research a European Network for Astrophysics [ARENA] | |
dc.contributor.author | SPINOGLIO, L. | |
dc.date.issued | 2018 | |
dc.identifier.issn | 1323-3580 | |
dc.description.abstractEn | The 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.iso | en | |
dc.publisher | Cambridge University Press (CUP) | |
dc.subject.en | Astrophysics - Astrophysics of Galaxies | |
dc.title.en | Probing the baryon cycle of galaxies with SPICA mid- and far-infrared observations | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1017/pasa.2017.67 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
dc.identifier.arxiv | 1711.11327 | |
bordeaux.journal | Publications of the Astronomical Society of Australia | |
bordeaux.page | id.e002 | |
bordeaux.volume | 35 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-01655546 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01655546v1 | |
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