Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/511
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dc.rights.licenseCopyright © 2021, Springer-Verlag GmbH Germany, part of Springer Nature-
dc.contributor.authorPérez Torres, M.-
dc.contributor.authorMattila, S.-
dc.contributor.authorAlonso Herrero, A.-
dc.contributor.authorAalto, S.-
dc.contributor.authorEfstathiou, A.-
dc.contributor.otherCentros de Excelencia Severo Ochoa, INSTITUTO DE ASTROFISICA DE ANDALUCIA (IAA), SEV-2017-0709-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2022-02-10T13:32:11Z-
dc.date.available2022-02-10T13:32:11Z-
dc.date.issued2021-01-13-
dc.identifier.citationThe Astronomy and Astrophysics Review 29(1): 2(2021)es
dc.identifier.issn0935-4956-
dc.identifier.otherhttps://link.springer.com/article/10.1007/s00159-020-00128-x-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/511-
dc.description.abstractNearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved studies of the interstellar medium, star formation and nuclear activity across a broad range of physical conditions. In particular, detailed studies of individual local luminous infrared galaxies (LIRGs) are crucial for gaining a better understanding of these processes and for developing and testing models that are used to explain statistical studies of large populations of such galaxies at high redshift for which it is currently impossible to reach a sufficient physical resolution. Here, we provide an overview of the impact of spatially resolved infrared, sub-millimetre and radio observations in the study of the interstellar medium, star formation and active galactic nuclei as well as their interplay in local LIRGs. We also present an overview of the modelling of their spectral energy distributions using state-of-the-art radiative transfer codes. These contribute necessary and powerful ‘workhorse’ tools for the study of LIRGs (and their more luminous counterparts) at higher redshifts which are unresolved in observations. We describe how spatially-resolved time-domain observations have recently opened a new window to study the nuclear activity in LIRGs. We describe in detail the observational characteristics of Arp 299 which is one of the best studied local LIRGs and exemplifies the power of the combination of time-domain and high-resolution observations at infrared to radio wavelengths together with radiative transfer modelling used to explain the spectral energy distributions of its different components. We summarise the previous achievements obtained using high-spatial resolution observations and provide an outlook into what we can expect to achieve with future facilities.es
dc.description.sponsorshipWe thank an anonymous referee for many useful comments and suggestions that have significantly improved our manuscript. We also thank Stuart Ryder for a careful reading of the whole paper, and Duncan Farrah, Erkki Kankare, Eskil Varenius and Naím Ramírez-Olivencia for comments on different sections of the paper. We also thank Naím Ramírez-Olivencia for the LOFAR image of Arp 299 in Fig. 25, in advance of publication, and Miguel Pereira-Santaella, Eric Murphy, and Eskil Varenius for producing new versions of their original figures (Figs. 4, 12-left, and 22-bottom, respectively). MPT acknowledges financial support from the State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709) and through grant PGC2018-098915-B-C21 (MCI/AEI/FEDER, UE) as well as from the visitor and mobility program of the Finnish Centre for Astronomy with ESO (FINCA), funded by the Academy of Finland grant nr 306531. AA-H acknowledges support through grant PGC 2018-094671-B-I00 (MCIU/AEI/FEDER, UE). AA-H work was done under project No. MDM-2017-0737 Unidad de Excelencia “María de Maeztu” - Centro de Astrobiología (INTA-CSIC). SA gratefully acknowledges support from an ERC Advanced Grant 789410 and from the Swedish Research Council. AE acknowledges support from the Cyprus Research & Innovation Foundation (GRATOS; EXCELLENCE/1216/0207) and the European Space Agency (CYGNUS; ESA contract 400126896/19/NL/MH).es
dc.language.isoenges
dc.publisherSpringer Linkes
dc.relationinfo:eu-repo/grantAgreement/ES/MCI-AEI-FEDER/PGC2018-098915-B-C21-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-094671-B-I00/ES/EVOLUCION DE GALAXIAS Y SUS AGUJEROS NEGROS CON ALTA RESOLUCION ESPACIAL: FEEDBACK, EL TORO Y FORMACION ESTELAR/-
dc.subjectGalaxieses
dc.subjectStarburstes
dc.subjectActivees
dc.subjectNucleies
dc.subjectISMes
dc.titleStar formation and nuclear activity in luminous infrared galaxies: an infrared through radio reviewes
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidPérez Torres, 0000-0001-5654-0266-
dc.identifier.doi10.1007/s00159-020-00128-x-
dc.identifier.e-issn1432-0754-
dc.contributor.funderEuropean Commission (EC)-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.contributor.funderMinisterio de Economía y Competitividad (MINECO)-
dc.description.peerreviewedPeerreviewes
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_dcae04bc-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/789410-
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