MOLYBDENUM AND RUTHENIUM ABUNDANCES IN COOL STARS OF THE GALACTIC DISC
Journal Title: Odessa Astronomical Publications - Year 2017, Vol 30, Issue
Abstract
We revise the molybdenum and ruthenium abundances in FGK stars with metallicities ranging from −1.0 < [Fe/H] < +0.3. The observed stars belong to the substructures of the Galaxy. The observations were conducted using the 1.93 m telescope at Observatoire de Haute-Provence (OHP, France) equipped with the echelle type spectrographs ELODIE and SOPHIE. The results are based on analyses of spectra that have a typical S/N ~ 100-300 and a resolution of 42 000. These estimates were obtained using synthetic spectra computed with LTE model atmosphere.
Authors and Affiliations
T. I. Gorbaneva, T. V. Mishenina
Keywords
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- EP ID EP348924
- DOI 10.18524/1810-4215.2017.30.114274
- Views 101
- Downloads 0
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