Chile | Articulo

Astronomy & Astrophysics

dc.creatorVillanova, S.
dc.creatorGeisler, D.
dc.date2020-03-11T20:36:46Z
dc.date2022-07-08T17:17:27Z
dc.date2020-03-11T20:36:46Z
dc.date2022-07-08T17:17:27Z
dc.date2011
dc.date.accessioned2023-08-22T04:57:22Z
dc.date.available2023-08-22T04:57:22Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/241085
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8322080
dc.descriptionContext. 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.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361/201117552
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleBimodality of light and s-elements in M4 (NGC 6121). A hint for the massive main-sequence star pollution scenario
dc.titleAstronomy & Astrophysics
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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