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Probing the cold magnetized Universe with SPICA-POL (B-BOP)

hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorANDRÉ, Ph.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorHUGHES, A.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorGUILLET, Vincent
dc.contributor.authorBOULANGER, F.
hal.structure.identifierIstituto Nazionale di Fisica Nucleare, Sezione di Milano [INFN]
dc.contributor.authorBRACCO, A.
dc.contributor.authorNTORMOUSI, E.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorARZOUMANIAN, D.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorMAURY, A. J.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorBERNARD, J.-Ph.
hal.structure.identifierFORMATION STELLAIRE 2019
dc.contributor.authorBONTEMPS, Sylvain
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorRISTORCELLI, I.
dc.contributor.authorGIRART, J. M.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorMOTTE, F.
dc.contributor.authorTASSIS, K.
hal.structure.identifierDépartement d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
dc.contributor.authorPANTIN, E.
dc.contributor.authorMONTMERLE, T.
hal.structure.identifierNatl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7 Canada
dc.contributor.authorJOHNSTONE, D.
hal.structure.identifierAstroParticule et Cosmologie [APC (UMR_7164)]
dc.contributor.authorGABICI, S.
dc.contributor.authorEFSTATHIOU, A.
hal.structure.identifierGroupement de Recherche et d'Etudes en Gestion à HEC [GREGH]
dc.contributor.authorBASU, S.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorBÉTHERMIN, M.
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorBEUTHER, H.
hal.structure.identifierFORMATION STELLAIRE 2019
dc.contributor.authorBRAINE, J.
hal.structure.identifierHerzberg Institute of Astrophysics
dc.contributor.authorDI FRANCESCO, J.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA (UMR_8112)]
dc.contributor.authorFALGARONE, E.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorFERRIÈRE, K.
dc.contributor.authorFLETCHER, A.
hal.structure.identifierUniversity of Cambridge [UK] [CAM]
dc.contributor.authorGALAMETZ, M.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorGIARD, M.
dc.contributor.authorHENNEBELLE, P.
dc.contributor.authorJONES, A.
dc.contributor.authorKEPLEY, A. A.
dc.contributor.authorKWON, J.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorLAGACHE, Guilaine
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA (UMR_8112)]
dc.contributor.authorLESAFFRE, Pierre
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA (UMR_8112)]
dc.contributor.authorLEVRIER, F.
hal.structure.identifierYangzhou University
dc.contributor.authorLI, D.
dc.contributor.authorLI, Z.-Y.
dc.contributor.authorMAO, S. A.
dc.contributor.authorNAKAGAWA, T.
dc.contributor.authorONAKA, T.
hal.structure.identifierAlma Mater Studiorum Università di Bologna = University of Bologna [UNIBO]
dc.contributor.authorPALADINO, R.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorPERETTO, N.
hal.structure.identifierMax Planck Institute for Extraterrestrial Physics [MPE]
dc.contributor.authorPOGLITSCH, A.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorREVERET, V.
hal.structure.identifierTelespazio
dc.contributor.authorRODRIGUEZ, L.
dc.contributor.authorSAUVAGE, M.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorSOLER, J. D.
hal.structure.identifierIstituto di Astrofisica e Planetologia Spaziali - INAF [IAPS]
dc.contributor.authorSPINOGLIO, L.
hal.structure.identifierInstitut für Physik [Potsdam]
dc.contributor.authorTABATABAEI, F.
dc.contributor.authorTRITSIS, A.
dc.contributor.authorVAN DER TAK, F.
hal.structure.identifierJeremiah Horrocks Institute for Mathematics, Physics and Astronomy [Preston]
dc.contributor.authorWARD-THOMPSON, D.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWIESEMEYER, H.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorYSARD, N.
dc.contributor.authorZHANG, H.
dc.date.issued2019
dc.identifier.issn1323-3580
dc.description.abstractEnSPICA, the cryogenic infrared space telescope recently pre-selected for a `Phase A' concept study as one of the three remaining candidates for ESA's fifth medium class (M5) mission, is foreseen to include a far-infrared polarimetric imager (SPICA-POL, now called B-BOP), which would offer a unique opportunity to resolve major issues in our understanding of the nearby, cold magnetized Universe. This paper presents an overview of the main science drivers for B-BOP, including high dynamic range polarimetric imaging of the cold interstellar medium (ISM) in both our Milky Way and nearby galaxies. Thanks to a cooled telescope, B-BOP will deliver wide-field 100-350 micron images of linearly polarized dust emission in Stokes Q and U with a resolution, signal-to-noise ratio, and both intensity and spatial dynamic ranges comparable to those achieved by Herschel images of the cold ISM in total intensity (Stokes I). The B-BOP 200 micron images will also have a factor ~30 higher resolution than Planck polarization data. This will make B-BOP a unique tool for characterizing the statistical properties of the magnetized interstellar medium and probing the role of magnetic fields in the formation and evolution of the interstellar web of dusty molecular filaments giving birth to most stars in our Galaxy. B-BOP will also be a powerful instrument for studying the magnetism of nearby galaxies and testing galactic dynamo models, constraining the physics of dust grain alignment, informing the problem of the interaction of cosmic rays with molecular clouds, tracing magnetic fields in the inner layers of protoplanetary disks, and monitoring accretion bursts in embedded protostars.
dc.language.isoen
dc.publisherCambridge University Press (CUP)
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enProbing the cold magnetized Universe with SPICA-POL (B-BOP)
dc.typeArticle de revue
dc.identifier.doi10.1017/pasa.2019.20
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1905.03520
bordeaux.journalPublications of the Astronomical Society of Australia
bordeaux.pagee029
bordeaux.volume36
bordeaux.peerReviewedoui
hal.identifierhal-02128417
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02128417v1
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