1. Dipòsit Digital de la Universitat de Barcelona
  2. Treballs de l'alumnat
  3. Treballs Finals de Grau (TFG) - Física
Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/59954
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dc.contributor.advisorJordi i Nebot, Carme-
dc.contributor.authorSanmartí, Enric-
dc.date.accessioned2014-11-24T10:51:03Z-
dc.date.available2014-11-24T10:51:03Z-
dc.date.issued2014-06-
dc.identifier.urihttp://hdl.handle.net/2445/59954-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2014, Tutora: Carme Jordica
dc.description.abstractThe purpose of this research is to determine the physical properties of an open cluster, including its age, using standard methodology. It is based on a photometric analysis of the stars in the area covered by the cluster, but astrometry is also needed to segregate cluster stars from eld stars. The colour-magnitude diagram is used for distance and age determination. The study focuses on NGC6405, a relatively young nearby open cluster.ca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Sanmartí, 2014-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/-
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationEstructura galàcticacat
dc.subject.classificationEstelscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherGalactic structureeng
dc.subject.otherStarseng
dc.subject.otherBachelor's theseseng
dc.titleThe Ages of Open Clusters: the Case of NGC6405eng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
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