LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud

dc.date.accessioned2020-03-11T20:35:57Z
dc.date.accessioned2022-10-18T23:02:18Z
dc.date.available2020-03-11T20:35:57Z
dc.date.available2022-10-18T23:02:18Z
dc.date.created2020-03-11T20:35:57Z
dc.date.issued2010
dc.identifierhttp://hdl.handle.net/10533/240807
dc.identifier15010003
dc.identifierWOS:000284625300012
dc.identifierno scielo
dc.identifiereid=2-s2.0-78649370523
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472146
dc.description.abstractContext. The amount of molecular gas is a key to understanding the future star formation in a galaxy. Because H2 is difficult to observe directly in dense and cold clouds, tracers such as the CO molecule are used. However, at low metallicities especially,
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361/200913372
dc.relation10.1051/0004-6361/200913372
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.titleLABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud
dc.typeArticulo


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