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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