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Magnesium abundance in the Galactic thick-disc stars and subsystem formation history

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The space velocities and Galactic orbital elements of stars calculated from the currently available high-accuracy observations in our compiled catalogue of spectroscopic magnesium abundances in dwarfs and subgiants in the solar neighbourhood are used to identify thick-disc objects. We analyse the relations between chemical, spatial and kinematic parameters of F–G stars in the identified subsystem.

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Keywords: Galactic evolution; Galaxy (Milky Way); Stellar chemical composition; Thick disc

Document Type: Research Article

Affiliations: 194 Stachki Street, Rostov-on-Don, 344090, Russia

Publication date: 01 April 2006

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