Magnesium abundance in the Galactic halo stars and subsystem formation history

Details Magnesium abundance in the Galactic halo stars and subsystem formation history Magnesium abundance in the Galactic halo stars and subsystem formation history

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26at...25..149m&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 25, Issue 2, p.149-152

Astronomy and Astrophysics

Astronomy

1

Galaxy (Milky Way), Stellar Chemical Composition, Halo Disc, Galactic Evolution

Scientific paper

Data from our compiled catalogue of spectroscopically determined magnesium abundances in dwarfs and subgiants with accurate parallaxes are used to select Galactic halo stars according to kinematic criteria and to identify presumably accreted stars among them. We analyse the relations between the relative magnesium abundances, metallicities and Galactic orbital elements for accreted halo stars.

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