Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations

During the past decade we have compiled a large molecular line data base of massive star forming regions in the southern Milky Way. These regions are confined into giant molecular clouds that trace the galactic spiral arms. Their radial distribution has a pronounced peak midway between the Sun and t...

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Detalles Bibliográficos
Autor: Bronfman, L.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2008
País:Chile
Idioma:inglés
OAI Identifier:oai:repositorio.anid.cl:10533/236920
Acceso en línea:https://hdl.handle.net/10533/236920
Access Level:acceso abierto
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spelling Bronfman, L.200810.1007/s10509-007-9597-2https://hdl.handle.net/10533/236920http://purl.org/coar/access_right/c_abf2Massive star formation in the southern Milky Way. From large scale surveys to high resolution observationsBronfman, L.2019-12-18T18:14:19Z2022-07-07T21:58:09Z2019-12-18T18:14:19Z2022-07-07T21:58:09Z2008During the past decade we have compiled a large molecular line data base of massive star forming regions in the southern Milky Way. These regions are confined into giant molecular clouds that trace the galactic spiral arms. Their radial distribution has a pronounced peak midway between the Sun and the galactic center, which in the IV quadrant corresponds to the location of the Norma Spiral arm. We study in some detail one of the foremost regions of massive star formation in the Norma arm, using millimeter continuum and line emission maps obtained with the SEST, APEX, and ASTE telescopes. It is a multiple system evolving along a complete GMC core, candidate for future ALMA observations.FONDAPFONDAP1501000315010003virtual::48341-1WOS:000252159900016https://hdl.handle.net/10533/236920enginstname: Conicytreponame: Repositorio Digital RI2.010.1007/s10509-007-9597-2info:eu-repo/grantAgreement/Fondap/15010003https://link.springer.com/article/10.1007/s10509-007-9597-2Atribución-NoComercial-SinDerivadas 3.0 Chilehttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/info:eu-repo/semantics/openAccessMassive star formation in the southern Milky Way. From large scale surveys to high resolution observationsAstrophysics & Space ScienceArticuloinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttps://hdl.handle.net/10533/236920http://purl.org/coar/resource_type/c_2df8fbb1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::48341-1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::48341-110533/236920oai:repositorio.anid.cl:10533/2369202023-07-24 19:38:09.942https://repositorio.anid.clRepositorio ANIDaletelier@anid.cl
dc.title.none.fl_str_mv Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
dc.title.journal.none.fl_str_mv Astrophysics & Space Science
title Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
spellingShingle Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
Bronfman, L.
title_short Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
title_full Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
title_fullStr Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
title_full_unstemmed Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
title_sort Massive star formation in the southern Milky Way. From large scale surveys to high resolution observations
dc.creator.none.fl_str_mv Bronfman, L.
author Bronfman, L.
author_facet Bronfman, L.
author_role author
description During the past decade we have compiled a large molecular line data base of massive star forming regions in the southern Milky Way. These regions are confined into giant molecular clouds that trace the galactic spiral arms. Their radial distribution has a pronounced peak midway between the Sun and the galactic center, which in the IV quadrant corresponds to the location of the Norma Spiral arm. We study in some detail one of the foremost regions of massive star formation in the Norma arm, using millimeter continuum and line emission maps obtained with the SEST, APEX, and ASTE telescopes. It is a multiple system evolving along a complete GMC core, candidate for future ALMA observations.
publishDate 2008
dc.date.issued.none.fl_str_mv 2008
dc.date.accessioned.none.fl_str_mv 2019-12-18T18:14:19Z
2022-07-07T21:58:09Z
dc.date.available.none.fl_str_mv 2019-12-18T18:14:19Z
2022-07-07T21:58:09Z
dc.type.none.fl_str_mv Articulo
dc.type.driver.none.fl_str_mv info:eu-repo/semantics/article
dc.type.openaire.none.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.folio.none.fl_str_mv 15010003
15010003
dc.identifier.idwos.none.fl_str_mv WOS:000252159900016
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/10533/236920
identifier_str_mv 15010003
WOS:000252159900016
url https://hdl.handle.net/10533/236920
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv instname: Conicyt
reponame: Repositorio Digital RI2.0
dc.relation.doi.none.fl_str_mv 10.1007/s10509-007-9597-2
dc.relation.projectid.none.fl_str_mv info:eu-repo/grantAgreement/Fondap/15010003
dc.relation.uri.none.fl_str_mv https://link.springer.com/article/10.1007/s10509-007-9597-2
dc.rights.none.fl_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rights.driver.none.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
eu_rights_str_mv openAccess
repository.name.fl_str_mv Repositorio ANID
repository.mail.fl_str_mv aletelier@anid.cl
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