Resolving the cosmic infrared background with the Herschel Space Observatory and dust destruction by radio jets.
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Date
2012
Authors
Journal Title
Journal ISSN
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Publisher
Universidad de Concepción
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.
Description
Tesis presentada para optar al grado de Doctor en Ciencias Físicas.
Keywords
Astronomía Infrarroja, Galaxias, Polvo Cósmico, Fotometría Astronómica.