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Doppler boosting effects on the radiation of relativistic jets in AGN

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dc.contributor Bosch i Ramon, Valentí
dc.creator Gil Pedret, Sergi
dc.date 2016-03-09T16:23:28Z
dc.date 2016-03-09T16:23:28Z
dc.date 2016-01
dc.date.accessioned 2024-12-16T10:22:10Z
dc.date.available 2024-12-16T10:22:10Z
dc.identifier http://hdl.handle.net/2445/96318
dc.identifier.uri http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/13899
dc.description Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: Valentí Bosch-Ramon
dc.description Active galactic nuclei are among the brightest sources in the Universe, with jets being detected in about a 10% of these objects. Studying the dynamics of these jets allows us to better understand the physics of these sources, and in particular why they are so powerful emitters. We model here the jets of active galactic nuclei as one dimensional supersonic relativistic fluids, assuming that they are described by the Bernoulli equation, plus a phenomenological prescription for their radius-height relation. With this model, we study the effects of relativistic Doppler boosting on the emitter structure and radiation intensity, which are sensitive to the viewing angle and radius-height jet relation
dc.format 5 p.
dc.format application/pdf
dc.language eng
dc.rights cc-by-nc-nd (c) Gil, 2016
dc.rights http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights info:eu-repo/semantics/openAccess
dc.source Treballs Finals de Grau (TFG) - Física
dc.subject Nucli galàctic actiu
dc.subject Radiació
dc.subject Treballs de fi de grau
dc.subject Active galactic nuclei
dc.subject Radiation
dc.subject Bachelor's theses
dc.title Doppler boosting effects on the radiation of relativistic jets in AGN
dc.type info:eu-repo/semantics/bachelorThesis


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