n-CAPTURE ELEMENTAL ABUNDANCES IN ACTIVE AND NON-ACTIVE STARS

dc.contributor.authorBasak, N. Yu.
dc.contributor.authorMishenina, T. V.
dc.contributor.authorSoubiran, C.
dc.contributor.authorKovtyukh, Valery V.
dc.contributor.authorBelik, S. I.
dc.date.accessioned2014-03-13T05:11:34Z
dc.date.available2014-03-13T05:11:34Z
dc.date.issued2010-07
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 07/2010 . – Vol.23.uk
dc.description.abstractAbundances of Y, Zr, La, Ce, Nd, and Sm have been obtained under LTE approximationss. The program stars were observed at high resolution, high signal to noise ratio with the ELODIE echelle spectrograph (OHP, France). Among them more than 30 stars are active stars with a fraction of BY Dra and RS CVn type stars. Comparison of the behavior of n-capture elemental abundance in active and non active stars was made.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4588
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 23, p. 17-18.
dc.subjectStars: fundamental parametersuk
dc.subjectstars: abundancesuk
dc.subjectstars: kinematicsuk
dc.subjectstars: atmospheresuk
dc.subjectGalaxy: stellar contentuk
dc.titlen-CAPTURE ELEMENTAL ABUNDANCES IN ACTIVE AND NON-ACTIVE STARSuk
dc.typeBookuk
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