Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?

Màster Oficial d'Astrofísica, Física de Partícules i Cosmologia, Facultat de Física, Universitat de Barcelona, Curs: 2015-2016, Tutors: Francesca Figueras, Teresa Antoja, Mercè Romero-Gómez, Santi Roca-Fàbrega

Detalles Bibliográficos
Autor: Reina Campos, Marta
Tipo de recurso: tesis de maestría
Fecha de publicación:2016
País:España
Institución:Universidad de Barcelona
Repositorio:Dipòsit Digital de la UB
OAI Identifier:oai:diposit.ub.edu:2445/147137
Acceso en línea:https://hdl.handle.net/2445/147137
Access Level:acceso abierto
Palabra clave:Galàxies
Via Làctia
Galàxia espiral
Treballs de fi de màster
Galaxies
Milky Way
Spiral galaxy
Master's theses
id ES_8622b71bb1355e3bfcdba5bf5e6c7b84
oai_identifier_str oai:diposit.ub.edu:2445/147137
network_acronym_str ES
network_name_str España
repository_id_str
spelling Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?Reina Campos, MartaGalàxiesVia LàctiaGalàxia espiralTreballs de fi de màsterGalaxiesMilky WaySpiral galaxyMaster's thesesMàster Oficial d'Astrofísica, Física de Partícules i Cosmologia, Facultat de Física, Universitat de Barcelona, Curs: 2015-2016, Tutors: Francesca Figueras, Teresa Antoja, Mercè Romero-Gómez, Santi Roca-FàbregaThe pattern speed of the non-axisymmetric structures of the galactic disc is a key parameter to understand the dynamics in the MilkyWay. For neither the Galactic bar nor the spiral arms it is well determined. All previous determinations have large uncertainties associated avoiding to shed some light on the nature of these structures.Figueras Siñol, FrancescaAntoja, T. (Teresa)Romero Gómez, MercèRoca Fàbrega, Santi2016info:eu-repo/semantics/masterThesisapplication/pdfhttps://hdl.handle.net/2445/147137Màster Oficial - Astrofísica, Física de Partícules i Cosmologiareponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaIngléscc-by-nc-nd (c) Reina, 2016http://creativecommons.org/licenses/by-nc-nd/3.0/es/info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/1471372026-05-27T06:46:51Z
dc.title.none.fl_str_mv Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
title Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
spellingShingle Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
Reina Campos, Marta
Galàxies
Via Làctia
Galàxia espiral
Treballs de fi de màster
Galaxies
Milky Way
Spiral galaxy
Master's theses
title_short Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
title_full Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
title_fullStr Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
title_full_unstemmed Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
title_sort Can the Tremaine - Weinberg method be used to determine the pattern speed of the bar and the spiral arms of the Milky Way?
dc.creator.none.fl_str_mv Reina Campos, Marta
author Reina Campos, Marta
author_facet Reina Campos, Marta
author_role author
dc.contributor.none.fl_str_mv Figueras Siñol, Francesca
Antoja, T. (Teresa)
Romero Gómez, Mercè
Roca Fàbrega, Santi
dc.subject.none.fl_str_mv Galàxies
Via Làctia
Galàxia espiral
Treballs de fi de màster
Galaxies
Milky Way
Spiral galaxy
Master's theses
topic Galàxies
Via Làctia
Galàxia espiral
Treballs de fi de màster
Galaxies
Milky Way
Spiral galaxy
Master's theses
description Màster Oficial d'Astrofísica, Física de Partícules i Cosmologia, Facultat de Física, Universitat de Barcelona, Curs: 2015-2016, Tutors: Francesca Figueras, Teresa Antoja, Mercè Romero-Gómez, Santi Roca-Fàbrega
publishDate 2016
dc.date.none.fl_str_mv 2016
dc.type.none.fl_str_mv info:eu-repo/semantics/masterThesis
format masterThesis
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/147137
url https://hdl.handle.net/2445/147137
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.rights.none.fl_str_mv cc-by-nc-nd (c) Reina, 2016
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv cc-by-nc-nd (c) Reina, 2016
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv Màster Oficial - Astrofísica, Física de Partícules i Cosmologia
reponame:Dipòsit Digital de la UB
instname:Universidad de Barcelona
instname_str Universidad de Barcelona
reponame_str Dipòsit Digital de la UB
collection Dipòsit Digital de la UB
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869412351936036864
score 15,300719

Similares en LA Referencia