Repositorio Dspace
Resolving the cosmic infrared background with the Herschel Space Observatory and dust destruction by radio jets.
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| dc.contributor.advisor | Nagar, Neil Mark; supervisor de grado | es |
| dc.contributor.author | Leiton-Thompson, Roger | es |
| dc.date.accessioned | 2020-12-22T18:37:35Z | |
| dc.date.available | 2020-12-22T18:37:35Z | |
| dc.date.issued | 2012 | |
| dc.identifier.uri | http://repositorio.udec.cl/jspui/handle/11594/1478 | |
| dc.description | Tesis presentada para obtener el grado de Doctor en Ciencias Físicas. | es |
| dc.description.abstract | During 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. | es |
| dc.language.iso | eng | es |
| dc.publisher | Universidad de Concepción. | es |
| dc.rights | Creative Commoms CC BY NC ND 4.0 internacional (Atribución-NoComercial-SinDerivadas 4.0 Internacional) | |
| dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/deed.es | |
| dc.source.uri | https://go.openathens.net/redirector/udec.cl?url=http://tesisencap.udec.cl/concepcion/leiton_r | |
| dc.subject | Astronomía Infrarroja | |
| dc.subject | Galaxias | |
| dc.subject | Polvo Cósmico | |
| dc.subject | Fotometría Astronómica. | |
| dc.title | Resolving the cosmic infrared background with the Herschel Space Observatory and dust destruction by radio jets. | es |
| dc.type | Tesis | es |
| dc.description.facultad | Facultad de Ciencias Físicas y Matemáticas | es |
| dc.description.departamento | Departamento de Astronomía. | es |
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