1999/03/22 by J. F. C. Santos Jr., J. F. C. Santos, A. E. Piatti +6 · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #History and Developments in Astronomy #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/300902
27 pages, 4 tables, 11 figures; accepted by the AJ
arxiv created 1999/03/22 · openalex publication_date 1999/06/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
A comparative analysis of Washington color-magnitude diagrams (CMDs) for 14 star clusters and respective surrounding fields in the Large Magellanic Cloud (LMC) outer disk is presented. Each CCD frame including field and the respective cluster covers an area of 185 arcmin 2 . The stellar population sampled is of intermediate age and metallicity. CMD radial analysis involving star count ratios, morphologies, and integrated light properties are carried out. Luminosity functions (LFs) are also presented. The two main results are, (1) within the range 4 kpc < R < 8 kpc, the distance from the LMC center is well correlated with the average age in the sense that inner fields are younger and (2) beyond ≈8 kpc the outer fields do not show evidence of a significant intermediate-age component in their stellar populations, as inferred from red giant clump star counts.