Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/9408
Title: The chemical composition of the active stars
Authors: Glazunova, L. V.
Citation: Odessa Astronomical Publications
Issue Date: 2016
Publisher: Одеський національний університет імені І. І. Мечникова
Keywords: Stars: RS CVn end BY Dra binaries
abundances – stars: individual: LX Per, OU Gem, BY Dra
Series/Report no.: ;V. 29
Abstract: The comparison of the results of the studies of the active stars’ chemical composition obtained by different authors has been performed. It was concluded that the difference between the abundances of some elements in active and inactive stars becomes significant (> 3 ) only for the active stars with high chromospheric activity (lgR′HK > 􀀀4). This is the case primarily for the light elements, namely Li, Na and Al, as well as heavy elements with Z > 30.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/9408
Appears in Collections:Odessa Astronomical Publications

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