Resolving the cosmic infrared background with the Herschel Space Observatory and dust destruction by radio jets.

dc.contributor.advisorNagar, Neil Markes
dc.contributor.authorLeiton-Thompson, Rogeres
dc.date.accessioned2020-12-22T18:37:35Z
dc.date.accessioned2024-05-15T16:30:23Z
dc.date.accessioned2024-08-28T22:40:21Z
dc.date.available2020-12-22T18:37:35Z
dc.date.available2024-05-15T16:30:23Z
dc.date.available2024-08-28T22:40:21Z
dc.date.issued2012
dc.descriptionTesis presentada para optar al grado de Doctor en Ciencias Físicas.es
dc.description.abstractDuring the last decades, infrared astronomy has changed our view about the evolution of galaxies, especially revealing that at large distances (z >1) individual galaxies are typically Utraluminous Infrared Galaxies (ULIRGs, 1012 < Lbol < 1013L.). Currently, we have access to large variety of physical information based on the emission in the infrared (IR) bands, radiation that in the case of galaxies mostly comes from dust grains.en
dc.description.campusConcepciónes
dc.description.departamentoDepartamento de Astronomíaes
dc.description.facultadFacultad de Ciencias Físicas y Matemáticases
dc.identifier.urihttps://repositorio.udec.cl/handle/11594/1478
dc.language.isoenen
dc.publisherUniversidad de Concepciónes
dc.rightsCC BY-NC-ND 4.0 DEED Attribution-NonCommercial-NoDerivs 4.0 Internationalen
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.source.urihttps://go.openathens.net/redirector/udec.cl?url=http://tesisencap.udec.cl/concepcion/leiton_r
dc.subjectAstronomía Infrarrojaes
dc.subjectGalaxiases
dc.subjectPolvo Cósmicoes
dc.subjectFotometría Astronómica.es
dc.titleResolving the cosmic infrared background with the Herschel Space Observatory and dust destruction by radio jets.en
dc.typeTesises

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