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dc.creatorNguyen-Luong, Q.
dc.creatorBronfman, L.
dc.date.accessioned2020-03-11T20:36:30Z
dc.date.available2020-03-11T20:36:30Z
dc.date.issued2011
dc.identifier.urihttp://hdl.handle.net/10533/240996
dc.description.abstractContext. In the framework of the multi-wavelength Galactic surveys of star-formation presently underway, complexes of molecular clouds that stretch over up to hundreds of parsecs are of particular interest. This is because a large population of stars is f
dc.language.isoeng
dc.relation.urihttps://doi.org/10.1051/0004-6361/201016271
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleW43: the closest molecular complex of the Galactic bar?
dc.typeArticulo
dc.identifier.folio15010003
dc.description.conicytprogramFONDAP
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.title.journalAstronomy & Astrophysics
dc.type.driverinfo:eu-repo/semantics/article
dc.description.shortconicytprogramFONDAP
dc.type.openaireinfo:eu-repo/semantics/publishedVersion


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