Analysis of hydrogen cyanide hyperfine spectral components towards star forming cores

dc.date.accessioned2020-03-11T20:36:39Z
dc.date.accessioned2022-10-18T23:04:15Z
dc.date.available2020-03-11T20:36:39Z
dc.date.available2022-10-18T23:04:15Z
dc.date.created2020-03-11T20:36:39Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/241061
dc.identifier15010003
dc.identifierWOS:000298717300010
dc.identifierno scielo
dc.identifiereid=2-s2.0-8485564928
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472400
dc.description.abstractAlthough hydrogen cyanide has become quite a common molecular tracing species for a variety of astrophysical sources, it, however, exhibits dramatic non-LTE behaviour in its hyperfine line structure. Individual hyperfine components can be strongly boosted
dc.languageeng
dc.relationhttps://arxiv.org/abs/1112.1743
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.titleAnalysis of hydrogen cyanide hyperfine spectral components towards star forming cores
dc.typeArticulo


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