For a sample of ~100 stars in M54 and the Sgr nucleus we give here: identifications, coordinates, BVIK magnitudes, heliocentric RV (table2); atmospheric parameters, [Fe/H] (table3); [O/Fe], [Na/Fe], [Mg/Fe], [Al/Fe] (table5); the α-elements Si, Ca, and Ti (table6); the Fe-peak elements Sc, V, Cr, Mn, Co, Ni, and Cu (table7).
Abundances of red giants in M54 and Sgr
LEONE, Francesco;
2010-01-01
Abstract
For a sample of ~100 stars in M54 and the Sgr nucleus we give here: identifications, coordinates, BVIK magnitudes, heliocentric RV (table2); atmospheric parameters, [Fe/H] (table3); [O/Fe], [Na/Fe], [Mg/Fe], [Al/Fe] (table5); the α-elements Si, Ca, and Ti (table6); the Fe-peak elements Sc, V, Cr, Mn, Co, Ni, and Cu (table7).File in questo prodotto:
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