Discovery of an Extremely High Velocity, Massive, and Compact Molecular Outflow in Norma

Astronomical Journal

dc.creatorBronfman, L.
dc.creatorGaray, G.
dc.creatorMardones, D.
dc.creatorMay, J.
dc.creatorMerello, M.
dc.date2020-03-11T20:26:43Z
dc.date2022-07-07T23:44:53Z
dc.date2020-03-11T20:26:43Z
dc.date2022-07-07T23:44:53Z
dc.date2008
dc.date.accessioned2023-08-23T00:19:13Z
dc.date.available2023-08-23T00:19:13Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/238104
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8354672
dc.descriptionG331.5–0.1 in the Norma spiral arm is one of the most luminous and extended cores of a giant molecular cloud (GMC), containing at least six massive and dense dust condensations. Here we report the discovery, from observations of several submillimeter mole
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1086/522487
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleDiscovery of an Extremely High Velocity, Massive, and Compact Molecular Outflow in Norma
dc.titleAstronomical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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