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http://hdl.handle.net/2445/147159
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DC Field | Value | Language |
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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.identifier.uri | http://hdl.handle.net/2445/147159 | - |
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.language.iso | eng | ca |
dc.rights | cc-by-nc-nd (c) Gutiérrez, 2017 | - |
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 |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | ca |
Appears in Collections: | Màster Oficial - Astrofísica, Física de Partícules i Cosmologia |
Files in This Item:
File | Description | Size | Format | |
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thesis_Carlos_Gutierrez.pdf | 3.42 MB | Adobe PDF | View/Open |
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