Manganes abundances in the atmosphere of clump giants

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dc.contributor.authorGorbanova, Tetiana I.en
dc.contributor.authorГорбаньова, Тетяна Іванівнаuk
dc.date.accessioned2014-03-23T03:37:22Z
dc.date.available2014-03-23T03:37:22Z
dc.date.issued2013
dc.description.abstractThe manganese abundances was determined in the atmospheres of clump giants stars whose selection was made earlier based on their chemical composition and evolutionary tracks. The spectra of the studied stars were obtained using the facilities of the 1.93 m telescope of the Haute-Provence Observatoire (France) equipped with the échelle spectrograph ELODIE (R = 42000, S/N = ~100–300). The Mn abundances was determined under the LTE approximation by the synthetic spectrum approach with a detailed consideration of the superfine structure. The behaviour of manganese abundances with metallicity [Fe/H] was considered.en
dc.identifier.citationOdessa Astronomical Publicationsen
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4754
dc.language.isoen
dc.publisherAstroprinten
dc.relation.ispartofseries;vol. 26, issue 1 , p. 60
dc.subjectstars: abundancesen
dc.titleManganes abundances in the atmosphere of clump giantsen
dc.typeArticleen
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Odesa Astronomical Publications