THREE GIANTS – MEMBERS OF THE OPEN CLUSTER M 67
Journal Title: Odessa Astronomical Publications - Year 2017, Vol 30, Issue
Abstract
We determined the atmospheric parameters and chemical composition of the three giants, which are members of the open cluster M 67. The high resolution spectra (R = 60 000) were obtained with the echelle spectrograph NES mounted on the 6-metertelescope of the SAO RAS Obtained variations in Na and Zr abundances are within the determination errors. The Li abundance suggest a depletion of Li in the course ofstellar evolution. For studied giants, the iron abundances derived from the neutral and ionized iron lines have not shown any significant discrepancies. The [Ba/Fe] values are close to the solar ones.
Authors and Affiliations
T. V. Mishenina, V. Klochkova, N. Basak, S. A. Korotin, A. Velichko
Keywords
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- EP ID EP349065
- DOI 10.18524/1810-4215.2017.30.114355
- Views 122
- Downloads 0
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