Chemical composition of stars in kinematical substructures of the galactic disk
Idioma
en
Communication dans un congrès
Este ítem está publicado en
2012EPJWC..1905006M - Assembling the Puzzle of the Milky Way, Le Grand-Bornand, France, Edited by C. Reylé; A. Robin; M. Schultheis; EPJ Web of Conferences, Volume 19, id.05006, 2012EPJWC..1905006M - Assembling the Puzzle of the Milky Way, Le Grand-Bornand, France, Edited by C. Reylé; A. Robin; M. Schultheis; EPJ Web of Conferences, Volume 19, id.05006, 2012, Le Grand-Bornand. 2012-02, vol. 19, p. 05006
Resumen en inglés
The Y, Zr, La, Ce, Nd , Sm and Eu abundances were found in LTE approach, and the abundance of Ba was computed in NLTE approximation for 280 FGK dwarfs in the region of metallicity of - 1<[Fe]< + 0.3. The selection of stars ...Leer más >