Characterizing filaments harboring high-mass star formation

Gutiérrez Chaves, Carlos Roberto

Characterizing filaments harboring high-mass star formation

dc.contributor.advisor	Busquet Rico, Gemma
dc.contributor.advisor	Estalella, Robert
dc.contributor.author	Gutiérrez Chaves, Carlos Roberto
dc.date.accessioned	2020-01-07T18:12:01Z
dc.date.available	2020-01-07T18:12:01Z
dc.date.issued	2017-09
dc.description	Màster Oficial d'Astrofísica, Física de Partícules i Cosmologia, Facultat de Física, Universitat de Barcelona, Curs: 2016-2017, Tutors: Gemma Busquet, Robert Estalella	ca
dc.description.abstract	A 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.extent	38 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/147159
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Gutiérrez, 2017
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.source	Màster Oficial - Astrofísica, Física de Partícules i Cosmologia
dc.subject.classification	Formació d'estels	cat
dc.subject.classification	Treballs de fi de màster	cat
dc.subject.classification	Stars formation	eng
dc.subject.other	Master's theses	eng
dc.title	Characterizing filaments harboring high-mass star formation	eng
dc.type	info:eu-repo/semantics/masterThesis	ca

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Màster Oficial - Astrofísica, Física de Partícules i Cosmologia