Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/171450
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dc.contributor.advisorAnders, Friedrich-
dc.contributor.advisorRomero Gómez, Mercè-
dc.contributor.authorTapial Rodríguez, Irene-
dc.date.accessioned2020-10-22T15:20:29Z-
dc.date.available2020-10-22T15:20:29Z-
dc.date.issued2020-06-
dc.identifier.urihttp://hdl.handle.net/2445/171450-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutors: Friedrich Anders, Mercè Romero-Gómezca
dc.description.abstractWe review some of the traits of the Galactic disc and elaborate on the Milky Way's Warp, the recent studies investigating it, and its importance. We focus on the effect of this distortion on different age populations using a broad sample of young objects made up by Cepheids, masers, and HII regions. We attempt a fit on this sample and compare it to other populations models available in the literature. We find less agreement with the similar age population OB model than expected, although some general trends are shared among all the models plotted. We also compare the positions of objects in our sample with respect to a HI Model, but find no evidence regarding a warping trend with age.ca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Tapial, 2020-
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.classificationVia Làctiacat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherGalaxies evolutioneng
dc.subject.otherMilky Wayeng
dc.subject.otherBachelor's theseseng
dc.titleThe evolution of the Galactic Warpeng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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