The growth of stellar discs in MW-like galaxies in TNG50

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dc.contributor.advisorLaporte, Chervin
dc.contributor.authorHidalgo Pifarré, Arnau
dc.date.accessioned2023-07-25T08:46:02Z
dc.date.available2023-07-25T08:46:02Z
dc.date.issued2023-06
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Chervin F. P. Laporteca
dc.description.abstractThe objective of this project has been to study the implications that a merger event has in the evolution of a galaxy, and whereas it can justify the formation of a thick disk akin to the one we observe in the Milky Way. In order to analyse this phenomena, we have looked at themetallicites, densities and velocity dispersion of the stellar population of a galactic disk for two galaxies; one which experienced a merger during its evolution and one that developed without. We also compared our results to those found in the literature in order to evaluate their validity, all while using available data from TNG50-1 simulation database.ca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/201125
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Hidalgo, 2023
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física
dc.subject.classificationEvolució de les galàxiescat
dc.subject.classificationDisc galàcticcat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherGalaxies evolutioneng
dc.subject.otherGalactic disceng
dc.subject.otherBachelor's theseseng
dc.titleThe growth of stellar discs in MW-like galaxies in TNG50eng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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Treballs Finals de Grau (TFG) - Física