Eu abundances in active and non-active stars

dc.contributor.author	Gorbanova, Tetiana I.	en
dc.contributor.author	Mishenina, Tamara V.	en
dc.contributor.author	Горбаньова, Тетяна Іванівна	uk
dc.contributor.author	Мішеніна, Тамара Василівна	uk
dc.date.accessioned	2014-03-13T05:35:27Z
dc.date.available	2014-03-13T05:35:27Z
dc.date.issued	2010-07
dc.description.abstract	Eu abundances have been determined for stars observed at high resolution, high signal to noise ratio with the ELODIE spectrograph at the 1.93-m telescope of the Observatoire de Haute Provence(France). Among them more than 30 stars are active stars with a fraction of BY Dra and RS CVn type stars for which spectral pecularities were investigated. For all stars fundamental parameters were determined earlier. We nd the mean abundances of the majority of elements in active and non-active stars. Active and non active cool dwarfs show similar dependencies of elemental ratios vs [Fe/H].	en
dc.identifier.citation	Odessa Astronomical Publications	en
dc.identifier.uri	https://dspace.onu.edu.ua/handle/123456789/4598
dc.language.iso	en
dc.publisher	Astroprint	en
dc.relation.ispartofseries	;vol. 23, p. 44-45.
dc.subject	stars: fundamental parameters	en
dc.subject	stars: Eu abundances	en
dc.title	Eu abundances in active and non-active stars	en
dc.type	Article	en

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