The Structure of a Low-metallicity Giant Molecular Cloud Complex

dc.date.accessioned2020-03-11T20:31:58Z
dc.date.accessioned2022-10-18T22:52:35Z
dc.date.available2020-03-11T20:31:58Z
dc.date.available2022-10-18T22:52:35Z
dc.date.created2020-03-11T20:31:58Z
dc.date.issued2009
dc.identifierhttp://hdl.handle.net/10533/239559
dc.identifier15010003
dc.identifierWOS:000269244500027
dc.identifierno scielo
dc.identifiereid=2-s2.0-70350608515
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4470898
dc.description.abstractTo understand the impact of low metallicities on giant molecular cloud (GMC) structure, we compare far-infrared dust emission, CO emission, and dynamics in the star-forming complex N83 in the Wing of the Small Magellanic Cloud (SMC). Dust emission (measur
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/702/1/352
dc.relation10.1088/0004-637X/702/1/352
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe Structure of a Low-metallicity Giant Molecular Cloud Complex
dc.typeArticulo


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