Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/4733
Title: LINES SELECTION TO DETERMINE THE CHEMICAL COMPOSITION OF STARS IN THE RANGE -3 ≤ [FE/H] ≤ -0.7
Authors: Basak, N. Yu.
Mishenina, T. V.
Citation: Odessa Astronomical Publications
Issue Date: 2012
Publisher: Astroprint
Keywords: abundance – Stars: late-type
Series/Report no.: ;vol. 25, issue 2, p.159
Abstract: ABSTRACT. Using the spectra obtained with echelle spectrograph SOPHIE (1.93 m telescope, OHP, France)and the data from about 20 papers of various authors, we have compiled a list for around four thousand lines of different chemical elements. Based on the spectra of the Sun and stars and also synthetic spectrum calculations in different ranges of metallicity, we selected 300 unblended lines of FeI, FeII and 200 lines of YII, ZrI, ZrII, LaII,CeII, PrII, NdII, SmII, GdII, that are recommended for thestudy of the chemical composition.
Description: Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2012 . – Vol.25/2.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/4733
Appears in Collections:Odessa Astronomical Publications

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