THE ABUNDANCES OF THE ELEMENTS OF THE MAGELLANIC CLOUDS

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dc.contributor.authorChekhonadskikh, F. A.
dc.date.accessioned2014-03-13T05:29:04Z
dc.date.available2014-03-13T05:29:04Z
dc.date.issued2010
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 07/2010 . – Vol.23.uk
dc.description.abstractThe results of the spectroscopic researches of classical Chepheids of the Magellanic Clouds (MC) are presented in this paper. 21 spectra for the Large Magellanic Cloud (LMC) and 10 for the Small Magellanic Cloud (SMC) were investigated. I obtained highly accurate values of e ective temperatures (Teff ), of the logarithm of the surface gravity(log g), of the microturbulence velocity (Vt), of abundances of elements for all of the objects. There is a good agreement with previous studies, some data were obtained for the rst time.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4595
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 23, p. 29-32.
dc.subjectClassical Cepheids: parameters of stellar athmosphereuk
dc.subjectMagellanic Clouds: abundancesuk
dc.titleTHE ABUNDANCES OF THE ELEMENTS OF THE MAGELLANIC CLOUDSuk
dc.typeArticleuk
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