N-capture elemental abundances in active and non-active stars

Скорочена інформація про документ
dc.contributor.authorBasak, Nina Yu.en
dc.contributor.authorMishenina, Tamara V.en
dc.contributor.authorSoubiran, C.en
dc.contributor.authorKovtyukh, Valery V.en
dc.contributor.authorBelik, S. I.en
dc.contributor.authorБасак, Ніна Юріївнаuk
dc.contributor.authorМішеніна, Тамара Василівнаuk
dc.contributor.authorКовтюх, Валерій Володимировичuk
dc.date.accessioned2014-03-13T05:11:34Z
dc.date.available2014-03-13T05:11:34Z
dc.date.issued2010-07
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.en
dc.identifier.citationOdessa Astronomical Publicationsen
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4588
dc.language.isoen
dc.publisherAstroprinten
dc.relation.ispartofseries;vol. 23, p. 17-18.
dc.subjectstars: fundamental parametersen
dc.subjectstars: abundancesen
dc.subjectstars: kinematicsen
dc.subjectstars: atmospheresen
dc.subjectGalaxy: stellar contenten
dc.titleN-capture elemental abundances in active and non-active starsen
dc.typeArticleen
Файли
Зібрання
Odesa Astronomical Publications