Europium abundances in cool dwarf stars of the galactic thick and thin disks

被引:1
作者
Gorbaneva, T. I. [1 ]
Mishenina, T. V. [1 ]
Soubiran, C. [2 ]
机构
[1] Odessa II Mechnikov State Univ, Astron Observ, UA-65014 Odessa, Ukraine
[2] Univ Bordeaux, Natl Ctr Sci Res, UMR 5804, F-33270 Floirac, France
基金
瑞士国家科学基金会;
关键词
EDGE-ON GALAXIES; NEUTRON-CAPTURE; VERTICAL-DISTRIBUTION; R-PROCESS; KINEMATICS; PARAMETERS; SPECTRA; ELODIE; TRENDS; HALO;
D O I
10.3103/S0884591312030038
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Abundances of europium for 112 FGK dwarf stars of thick and thin disks have been determined in the metallicity range of -1.0 < [Fe/H] < +0.3. Spectra of the studied stars have been obtained using the 1.93-m telescope of Haute-Provence Observatory (France) with spectral resolution R = 42000 and signal-to-noise ratio S/N = 100-300. Eu content has been calculated with assumption of LTE using the synthetic spectrum approach with detailed consideration of superfine structure. Analysis of europium abundances as a function of metallicity in kinematically selected stars of the Galactic thick and thin disks revealed different values in the disks. Comparison of europium abundances with magnesium abundances makes it possible to assume that at [Fe/H] < -0.2 dex the origins of these elements are similar and at [Fe/H] > -0.2 dex they are, probably, different.
引用
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页码:121 / 127
页数:7
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