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Cited article:
E. Bica, S. Ortolani, B. Barbuy
Astron. Astrophys. Suppl. Ser., 136 2 (1999) 363-372
Published online: 1999-04-15
This article has been cited by the following article(s):
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Classifying Globular Clusters and Applying them to Estimate the mass of the Milky Way
GuangChen Sun, Yougang Wang, Chao Liu, Richard J. Long, Xuelei Chen and Qi Gao
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The Evolution of The Milky Way
Randy L. Phelps
Astrophysics and Space Science Library, The Evolution of The Milky Way 255 239 (2000)
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Structural parameters of 11 faint Galactic globular clusters derived with 2MASS
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CCD Photometry of the Old Clusters ESO 093-SC08 and van den Bergh-Hagen 176
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The Astronomical Journal 126 (1) 265 (2003)
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ESO 452−SC11: the lowest mass globular cluster with a potential chemical inhomogeneity
Jeffrey D. Simpson, Gayandhi De Silva, Sarah L. Martell, Colin A. Navin and Daniel B. Zucker
Monthly Notices of the Royal Astronomical Society 472 (3) 2856 (2017)
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Dissolving star cluster candidates
E. Bica, B. X. Santiago, C. M. Dutra, et al.
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Colour Magnitude Diagrams of the moderately metal-rich globular
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S. Ortolani, E. Bica and B. Barbuy
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Gaia EDR3 view on galactic globular clusters
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A. D. Mackey and G. F. Gilmore
Monthly Notices of the Royal Astronomical Society 355 (2) 504 (2004)
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CCD Photometry of the Globular Cluster ESO 452-SC11
Alexis S. M. Cornish, Randy L. Phelps, Michael M. Briley and Eileen D. Friel
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Detailed chemical abundance analysis of the thick disk star cluster Gaia 1
Andreas Koch, Terese T. Hansen and Andrea Kunder
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An analysis of the most distant cataloged open clusters
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Globular Cluster as Indicators of Galactic Evolution
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Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST, and literature data
H Baumgardt and E Vasiliev
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