dc.date.accessioned2018-12-07T13:33:41Z
dc.date.accessioned2022-10-18T21:59:44Z
dc.date.available2018-12-07T13:33:41Z
dc.date.available2022-10-18T21:59:44Z
dc.date.created2018-12-07T13:33:41Z
dc.date.issued2016
dc.identifierhttp://hdl.handle.net/10533/232666
dc.identifier1151239
dc.identifierWOS:000373741300037
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4464021
dc.description.abstractIn this paper, we report our high-resolution (0 ''.20 x 0 ''.14 or similar to 70 x 49 pc) observations of the CO(6-5) line emission, which probes warm and dense molecular gas, and the 434 mu m dust continuum in the nuclear region of NGC 7130, obtained wit
dc.languageeng
dc.relationhttp://iopscience.iop.org/article/10.3847/0004-637X/820/2/118/meta
dc.relationhandle/10533/111557
dc.relation10.3847/0004-637X/820/2/118
dc.relationhandle/10533/111541
dc.relationhandle/10533/108045
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.titleAlma Imaging Of The Co (6-5) Line Emission In Ngc 7130
dc.typeArticulo


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