The first chemical abundance analysis of K giants in the inner Galactic disc

dc.date.accessioned2020-03-11T20:35:31Z
dc.date.accessioned2022-10-18T23:01:05Z
dc.date.available2020-03-11T20:35:31Z
dc.date.available2022-10-18T23:01:05Z
dc.date.created2020-03-11T20:35:31Z
dc.date.issued2010
dc.identifierhttp://hdl.handle.net/10533/240648
dc.identifier15010003
dc.identifierWOS:000280275400013
dc.identifierno scielo
dc.identifiereid=2-s2.0-77957552446
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4471987
dc.description.abstractAims. The elemental abundance structure of the Galactic disc has been extensively studied in the solar neighbourhood using long-lived stars such as F and G dwarfs or K and M giants. These are stars whose atmospheres preserve the chemical composition of th
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361/201014809
dc.relation10.1051/0004-6361/201014809
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.titleThe first chemical abundance analysis of K giants in the inner Galactic disc
dc.typeArticulo


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