2005/05/05 by E. Valenti, L. Origlia, F. R. Ferraro · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Bulge #Galaxy #Globular cluster #Metallicity #Open cluster #Photometric system #Photometry (optics) #Physics #Red-giant branch #Star cluster #Stars #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1111/j.1365-2966.2005.09173.x
published as Mon.Not.Roy.Astron.Soc. 361 (2005) 272-282 · 12 pages, 15 figures, accepted for publication in MNRAS
arxiv created 2005/05/05 · openalex publication_date 2005/07/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present high-quality near-infrared (near-IR) photometry of four bulge metal-rich globular clusters, namely NGC 6304, 6569, 6637 and 6638. By using the observed colour—magnitude diagrams we derived photometric estimates of the cluster reddening and distance. We performed a detailed analysis of the red giant branch (RGB), presenting a complete description of its morphologic parameters and evolutionary features (bump and tip). Photometric estimates of the cluster metallicity were obtained using the updated data set (published by our group) linking metal abundance to a variety of near-IR indices measured along the RGB. The detection of the RGB bump and tip is also presented and briefly discussed.