Manganes abundances in the atmosphere of clump giants

dc.contributor.author	Gorbanova, Tetiana I.	en
dc.contributor.author	Горбаньова, Тетяна Іванівна	uk
dc.date.accessioned	2014-03-23T03:37:22Z
dc.date.available	2014-03-23T03:37:22Z
dc.date.issued	2013
dc.description.abstract	The 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.citation	Odessa Astronomical Publications	en
dc.identifier.uri	https://dspace.onu.edu.ua/handle/123456789/4754
dc.language.iso	en
dc.publisher	Astroprint	en
dc.relation.ispartofseries	;vol. 26, issue 1 , p. 60
dc.subject	stars: abundances	en
dc.title	Manganes abundances in the atmosphere of clump giants	en
dc.type	Article	en