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The Ital-FLAMES survey of the Sagittarius dwarf spheroidal galaxy

2005/06/30 by L. Monaco, M. Bellazzini, P. Bonifacio +5 · 154 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Dwarf galaxy #Dwarf spheroidal galaxy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Giant star #Interacting galaxy #Metallicity #Milky Way #Physics #Sagittarius #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20053333

published in Astronomy and Astrophysics 441(1), 141-151 (EDP Sciences) · 16 pages, 10 figures, 6 tables. Accepted for publication in A&A. Minor changes in the text

openalex publication_date 2005/09/13 · arxiv created 2005/10/02 · arxiv updated 2016/08/30 · openalex created_date 2022/10/03 · openalex updated_date 2026/07/31

Abstract

We present iron and α element (Mg, Ca, Ti) abundances for a sample of 15 Red Giant Branch stars belonging to the main body of the Sagittarius dwarf Spheroidal galaxy. Abundances have been obtained from spectra collected using the high resolution spectrograph FLAMES-UVES mounted at the VLT. Stars of our sample have a mean metallicity of [ Fe/H with a metal-poor tail extending to [ Fe/H. The α element abundance ratios are slightly subsolar for metallicities higher than , suggesting a slow star formation rate. The [ α/Fe] of stars having are compatible to what observed in Milky Way stars of comparable metallicity.

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