The Ages of Open Clusters: the Case of NGC6405

dc.contributor.advisor	Jordi i Nebot, Carme
dc.contributor.author	Sanmartí, Enric
dc.date.accessioned	2014-11-24T10:51:03Z
dc.date.available	2014-11-24T10:51:03Z
dc.date.issued	2014-06
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2014, Tutora: Carme Jordi	ca
dc.description.abstract	The 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.extent	5 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/59954
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Sanmartí, 2014
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	Estructura galàctica	cat
dc.subject.classification	Estels	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Galactic structure	eng
dc.subject.other	Stars	eng
dc.subject.other	Bachelor's theses	eng
dc.title	The Ages of Open Clusters: the Case of NGC6405	eng
dc.type	info:eu-repo/semantics/bachelorThesis	ca

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