Bimodality of light and s-elements in M4 (NGC 6121). A hint for the massive main-sequence star pollution scenario

dc.date.accessioned2020-03-11T20:36:46Z
dc.date.accessioned2022-10-18T23:04:25Z
dc.date.available2020-03-11T20:36:46Z
dc.date.available2022-10-18T23:04:25Z
dc.date.created2020-03-11T20:36:46Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/241085
dc.identifier15010003
dc.identifierWOS:000297841200043
dc.identifierno scielo
dc.identifiereid=2-s2.0-80555156827
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472424
dc.description.abstractContext. All globular clusters (GCs) studied in detail host two or more populations of stars (the multiple population phenomenon). Theoretical models suggest that the second population is formed from gas polluted by processed material produced by massive
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361/201117552
dc.relation10.1051/0004-6361/201117552
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.titleBimodality of light and s-elements in M4 (NGC 6121). A hint for the massive main-sequence star pollution scenario
dc.typeArticulo


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