OGLE SMC-ECL- 6249 , the SIMBAD biblio

OGLE SMC-ECL- 6249 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST08:54:39


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Title First 3 Authors
2016AcA....66..421P viz 16       D               1 48605 77 The OGLE Collection of Variable Stars. Eclipsing Binaries in the Magellanic System. PAWLAK M., SOSZYNSKI I., UDALSKI A., et al.
2020MNRAS.492.4254T 3334   K A D S   X C       80 8 ~ The Cluster AgeS Experiment (CASE) - VIII. Age and distance of the Globular Cluster 47 Tuc from the analysis of two detached eclipsing binaries. THOMPSON I.B., UDALSKI A., DOTTER A., et al.
2021ApJS..255....1B viz 17       D               1 498270 9 Classification of OGLE eclipsing binary stars based on their morphology type with locally linear embedding. BODI A. and HAJDU T.
2022MNRAS.509.4208V 213           X C F     3 16 4 Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si. II. Application to the colour-magnitude diagrams of the globular clusters 47 Tuc, NGC 6362, M 5, M 3, M 55, and M92. VANDENBERG D.A., CASAGRANDE L. and EDVARDSSON B.
2022MNRAS.517.2485R 85           X         2 10 1 The Cluster Ages Experiment (CASE) - IX. Analysis of four detached eclipsing binaries in the globular cluster NGC 3201. ROZYCZKA M., THOMPSON I.B., DOTTER A., et al.
2023AJ....165...30X viz 17       D               1 185 3 The Eclipsing Binaries from the LAMOST Medium-resolution Survey. III. A High-precision Empirical Stellar Mass Library. XIONG J., LIU C., LI J., et al.
2023MNRAS.518.4517V 44           X         1 15 2 Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si - III. Grids of isochrones for -2.5 ≤ [Fe/H] ≤ -0.5 and helium abundances Y = 0.25 and 0.29 at each metallicity. VANDENBERG D.A.
2024A&A...691A.166C 179           X         4 3 ~ Relative evolution of eclipsing binaries: A tool for measuring globular cluster ages and He abundances. CRISTI-CAMBIASO N., CATELAN M., VALCARCE A.A.R., et al.
2025MNRAS.539.3741M 19       D               1 103 ~ Benchmark stars for mean stellar density and surface gravity estimates of solar-type stars. MAXTED P.F.L.

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