2011/03/31 by O. A. Gonzalez, O. A. González, M. Rejkuba +12 · 4 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Bulge #Galaxy #Giant star #Globular cluster #Halo #Metallicity #Milky Way #Physics #Red-giant branch #Spectral line #Stars #Stellar, planetary, and galactic studies #Thick disk #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201116548
13 pages, 17 figures. Accepted for publication in Astronomy and Astrophysics
arxiv created 2011/03/31 · openalex publication_date 2011/04/11 · arxiv updated 2015/05/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Aims. We present the analysis of the [α/Fe] abundance ratios for a large number of stars at several locations in the Milky Way bulge with the aim of constraining its formation scenario.