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

dc.contributor.advisor	Salvador Solé, Eduard
dc.contributor.author	Colom Bernadich, Miquel
dc.date.accessioned	2018-09-27T15:55:44Z
dc.date.available	2018-09-27T15:55:44Z
dc.date.issued	2018-06
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Eduard Salvador Solé	ca
dc.description.abstract	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.	ca
dc.format.extent	5 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/124897
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Colom, 2018
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.source	Treballs Finals de Grau (TFG) - Física
dc.subject.classification	Formació de les galàxies	cat
dc.subject.classification	Nucli galàctic actiu	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Galaxy formation	eng
dc.subject.other	Active galactic nuclei	eng
dc.subject.other	Bachelor's theses	eng
dc.title	Implementation of the radio/jet mode AGN feedback in the AMIGA model	eng
dc.type	info:eu-repo/semantics/bachelorThesis	ca

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