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dc.contributor.authorParamonova, O. P.-
dc.contributor.authorMishenina, T. V.-
dc.contributor.authorChepizhko, O.-
dc.date.accessioned2014-03-28T07:43:49Z-
dc.date.available2014-03-28T07:43:49Z-
dc.date.issued2013-
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/4779-
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2013 . – Vol.26/1.uk
dc.description.abstractThe sulfur abundance was determined by the synthetic spectrum method in the stars with metallicity close to that of the Sun. The comparison with the results of other authors, as well as the nucleosynthesis computations were made.uk
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 26, issue 1, p. 94-
dc.subjectStarsuk
dc.subjectabundance – Starsuk
dc.subjectlate-typeuk
dc.titleSULFUR ABUNDANCE IN THE GALACTIC DISC STARSuk
dc.typeArticleuk
Appears in Collections:Odessa Astronomical Publications

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