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Mg, Ba and Eu abundances in thick disk and halo starsOur sample of cool dwarf stars from previous papers (Mashonkina & Gehren 2000, 2001) is extended

Heavy element abundances in cool dwarf stars: An implication for the evolution of the Galaxy in our previous analysis (Mashonkina & Gehren 2000) is confirmed in this study: [Eu/Ba] and [Eu

Barium abundances in cool dwarf stars as a constraint to s- and r-process nucleosynthesis

Barium abundances in cool dwarf stars as a constraint to s- and r-process nucleosynthesis

Barium and europium abundances in cool dwarf stars and nucleosynthesis of heavy elements

Mg, Ba and Eu abundances in thick disk and halo starsOur sample of cool dwarf stars from previous papers (Mashonkina & Gehren 2000, 2001) is extended

Heavy element abundances in cool dwarf stars: An implication for the evolution of the Galaxy in our previous analysis (Mashonkina & Gehren 2000) is confirmed in this study: [Eu/Ba] and [Eu

Barium and europium abundances in cool dwarf stars and nucleosynthesis of heavy elements

40 ЛЕТ КАЗАНСКОЙ ШКОЛЕ НЕ-ЛТР-ИССЛЕДОВАНИЙ: ДОСТИЖЕНИЯ И ПРОБЛЕМЫ // Ученые записки КФУ. Физико-математические науки 2011 N2

ОБОГАЩЕНИЕ ЭЛЕМЕНТАМИ НЕЙТРОННОГО ЗАХВАТА ЗВЕЗД ТОНКОГО И ТОЛСТОГО ДИСКОВ ГАЛАКТИКИ // Ученые записки КФУ. Физико-математические науки 2011 N2

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