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dc.creatorCovarrubias, R.
dc.creatorDalcanton, J.
dc.creatorHamuy, M.
dc.date.accessioned2020-08-04T21:51:02Z
dc.date.available2020-08-04T21:51:02Z
dc.date.issued2005
dc.identifier.urihttp://hdl.handle.net/10533/242585
dc.description.abstractWe are working to answer this question by measuring abundances of HII regions in galaxies that hosted Core Collapse Supernovae (CCSNe), and correlating them with the SN properties. The latter will be derived for 63 nearby (z < 0.08) CCSNe with high qualit
dc.language.isoeng
dc.relationinstname: ANID
dc.relationreponame: Repositorio Digital RI2.0
dc.relation.urihttps://www.researchgate.net/publication/260256915_Does_Metallicity_Affect_the_Fate_of_Massive_Stars
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleDoes Metallicity Affect the Fate of Massive Stars?
dc.typeCapitulo de libro
dc.identifier.folio15010003
dc.description.conicytprogramFONDAP
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.type.driverinfo:eu-repo/semantics/bookPart
dc.description.shortconicytprogramFONDAP
dc.title.libroAmerican Astronomical Society Meeting
dc.description.centroCENASTRO


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