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Implementation of the radio/jet mode AGN feedback in the AMIGA model

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dc.contributor Salvador Solé, Eduard
dc.creator Colom Bernadich, Miquel
dc.date 2018-09-27T15:55:44Z
dc.date 2018-09-27T15:55:44Z
dc.date 2018-06
dc.date.accessioned 2024-12-16T10:26:44Z
dc.date.available 2024-12-16T10:26:44Z
dc.identifier http://hdl.handle.net/2445/124897
dc.identifier.uri http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/21475
dc.description Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Eduard Salvador Solé
dc.description In this Treball de Fi de Grau the radio/jet mode Active Galactic Nunclei reheating feedback has been implemented in the AMIGA model, a semi-analytic hierarchical model of galaxy formation that works in the [Delta]CDM cosmology, in order to observe its possible repercussions onthe galaxy and black hole mass functions at redshifts z = 6:3 and z = 3:9 for the cases of radio/jet mode effciency equal to 0:1 and 1.
dc.format 5 p.
dc.format application/pdf
dc.language eng
dc.rights cc-by-nc-nd (c) Colom, 2018
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 Formació de les galàxies
dc.subject Nucli galàctic actiu
dc.subject Treballs de fi de grau
dc.subject Galaxy formation
dc.subject Active galactic nuclei
dc.subject Bachelor's theses
dc.title Implementation of the radio/jet mode AGN feedback in the AMIGA model
dc.type info:eu-repo/semantics/bachelorThesis


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