Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/171394
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dc.contributor.advisorAnders, Friedrich-
dc.contributor.authorQuadrino Lodoso, Irene-
dc.date.accessioned2020-10-22T12:30:35Z-
dc.date.available2020-10-22T12:30:35Z-
dc.date.issued2020-06-
dc.identifier.urihttp://hdl.handle.net/2445/171394-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Friedrich Andersca
dc.description.abstractOur galaxy contains a large number of stellar open clusters still to be identified and characterized, but thanks to the new Gaia DR2 release, it is possible to identify new ones that are unknown to date and discard earlier reported clusters that turn out to be spurious. The aim of this work is to do a statistical analysis of the spatial and the age distribution as well as the completeness, using the most recent and comprehensive sample of open clusters available today from the Gaia satellite. Using these data and comparing them with old catalogues, we redetermine fundamental parameters of the cluster age function: logTbreak=8.52±0.18 ,α1=−0.61±0.28, α2=−1.82±0.15 for the broken power-law fit and logT∗=8.89±0.15, αT=−0.55±0.10 for the Schechter fit.ca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Quadrino, 2020-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationCúmuls de galàxiescat
dc.subject.classificationVia Làctiacat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherClusters of galaxieseng
dc.subject.otherMilky Wayeng
dc.subject.otherBachelor's theseseng
dc.titleOpen clusters and the structure of the Milky Wayeng
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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