Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/147159
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dc.contributor.advisorBusquet Rico, Gemma-
dc.contributor.advisorEstalella, Robert-
dc.contributor.authorGutiérrez Chaves, Carlos Roberto-
dc.date.accessioned2020-01-07T18:12:01Z-
dc.date.available2020-01-07T18:12:01Z-
dc.date.issued2017-09-
dc.identifier.urihttp://hdl.handle.net/2445/147159-
dc.descriptionMàster Oficial d'Astrofísica, Física de Partícules i Cosmologia, Facultat de Física, Universitat de Barcelona, Curs: 2016-2017, Tutors: Gemma Busquet, Robert Estalellaca
dc.description.abstractA distinguished kind of molecular clouds, the infrared dark clouds (hereafter IRDCs), are believed to be relevant for describing the initial conditions for high-mass star formation. They are characterized by their lack of detectable emission in the mid-infrared: they appear as a dark silhouette against the corresponding mid-infrared background. IRDCs were first recognized in images from the Infrared Space Observatory (ISO, Egan et al. 1998) and the Midcourse Space Experiment (MSX, Perault et al. 1996)ca
dc.format.extent38 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Gutiérrez, 2017-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceMàster Oficial - Astrofísica, Física de Partícules i Cosmologia-
dc.subject.classificationFormació d'estelscat
dc.subject.classificationTreballs de fi de màstercat
dc.subject.classificationStars formationeng
dc.subject.otherMaster's theseseng
dc.titleCharacterizing filaments harboring high-mass star formationeng
dc.typeinfo:eu-repo/semantics/masterThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
Appears in Collections:Màster Oficial - Astrofísica, Física de Partícules i Cosmologia

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