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/2445/188959
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dc.contributor.advisorBusquet Rico, Gemma-
dc.contributor.authorTorres Duran, Eduard-
dc.date.accessioned2022-09-12T13:15:55Z-
dc.date.available2022-09-12T13:15:55Z-
dc.date.issued2022-06-
dc.identifier.urihttp://hdl.handle.net/2445/188959-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutora: Gemma Busquet Ricoca
dc.description.abstractWe obtained images of the G14.2 Hub-S with data acquired by ALMA. The visibilities were weighted naturally and with robust=0 with the task tclean of CASA to get different spatial resolutions (160 and 64 AU, respectively). We identified 22 sources with the tool PyBDSF and we estimated their masses and sizes. We found that most of the sources correspond to low-mass protostellar disks but there is a large mass reservoir in the envelope that can feed the protostar to become high-mass starsca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Torres, 2022-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationNúvol fosc infraroigcat
dc.subject.classificationCúmuls de galàxiescat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherInfrared dark cloudeng
dc.subject.otherClusters of galaxieseng
dc.subject.otherBachelor's theseseng
dc.titleFragmentation and cluster formation in the Infrared Dark Cloud G14.225−0.506eng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
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