Comparisons of the radial distributions of core-collapse supernovae with those of young and old stellar populations

dc.date.accessioned2020-03-11T20:32:59Z
dc.date.accessioned2022-10-18T22:54:55Z
dc.date.available2020-03-11T20:32:59Z
dc.date.available2022-10-18T22:54:55Z
dc.date.created2020-03-11T20:32:59Z
dc.date.issued2009
dc.identifierhttp://hdl.handle.net/10533/239859
dc.identifier15010003
dc.identifierWOS:000270661300005
dc.identifierno scielo
dc.identifiereid=2-s2.0-70349878833
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4471198
dc.description.abstractWe present observational constraints on the nature of core-collapse supernovae through an investigation into their radial distributions with respect to those of young and old stellar populations within their host galaxies, as traced by H-alpha emission an
dc.languageeng
dc.relationhttps://doi.org/10.1111/j.1365-2966.2009.15324.x
dc.relation10.1111/j.1365-2966.2009.15324.x
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.titleComparisons of the radial distributions of core-collapse supernovae with those of young and old stellar populations
dc.typeArticulo


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