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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
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Models of metal-poor stars with different initial abundances of C, N, O, Mg, and Si – I. Bolometric corrections derived from new MARCS synthetic spectra and their implications for observed colour–magnitude diagrams
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Properties of the brightest globular cluster in M 81 based on multicolour observations
On the determination of the He abundance distribution in globular clusters from the width of the main sequence
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Yonsei Evolutionary Population Synthesis (YEPS). II. Spectro-photometric Evolution of Helium-enhanced Stellar Populations
THE HUBBLE SPACE TELESCOPE UV LEGACY SURVEY OF GALACTIC GLOBULAR CLUSTERS. VII. IMPLICATIONS FROM THE NEARLY UNIVERSAL NATURE OF HORIZONTAL BRANCH DISCONTINUITIES*
T. M. Brown, S. Cassisi, F. D’Antona, M. Salaris, A. P. Milone, E. Dalessandro, G. Piotto, A. Renzini, A. V. Sweigart, A. Bellini, S. Ortolani, A. Sarajedini, A. Aparicio, L. R. Bedin, J. Anderson, A. Pietrinferni and D. Nardiello The Astrophysical Journal 822(1) 44 (2016) https://doi.org/10.3847/0004-637X/822/1/44
Spiral arm kinematics for Milky Way stellar populations
Stellar models of multiple populations in globular clusters – I. The main sequence of NGC 6752
Aaron Dotter, Jason W. Ferguson, Charlie Conroy, et al. Monthly Notices of the Royal Astronomical Society 446(2) 1641 (2015) https://doi.org/10.1093/mnras/stu2170
On the nature of the brightest globular cluster in M81
Y. D. Mayya, D. Rosa-González, M. Santiago-Cortés, et al. Monthly Notices of the Royal Astronomical Society 436(3) 2763 (2013) https://doi.org/10.1093/mnras/stt1784
STAR FORMATION HISTORIES OF GLOBULAR CLUSTERS WITH MULTIPLE POPULATIONS. I. ω CEN, M22, AND NGC 1851
WIYN OPEN CLUSTER STUDY. XXXIX. ABUNDANCES IN NGC 6253 FROM HYDRA SPECTROSCOPY OF THE Li 6708 Å REGION
Barbara J. Anthony-Twarog, Constantine P. Deliyannis, Bruce A. Twarog, Jeffrey D. Cummings and Ryan M. Maderak The Astronomical Journal 139(5) 2034 (2010) https://doi.org/10.1088/0004-6256/139/5/2034
HOT HORIZONTAL BRANCH STARS IN ω CENTAURI: CLUES ABOUT THEIR ORIGIN FROM THE CLUSTER COLOR MAGNITUDE DIAGRAM
Globular clusters as laboratories for stellar evolution
Márcio Catelan, Aldo A. R. Valcarce and Allen V. Sweigart Proceedings of the International Astronomical Union 5(S266) 281 (2009) https://doi.org/10.1017/S1743921309991153
A LARGE SAMPLE STUDY OF RED GIANTS IN THE GLOBULAR CLUSTER OMEGA CENTAURI (NGC 5139)
Aaron Dotter, Brian Chaboyer, Darko Jevremović, et al. The Astrophysical Journal Supplement Series 178(1) 89 (2008) https://doi.org/10.1086/589654
The helium abundance and ΔY/ΔZ in lower main-sequence stars
Luca Casagrande, Chris Flynn, Laura Portinari, Leo Girardi and Raul Jimenez Monthly Notices of the Royal Astronomical Society 382(4) 1516 (2007) https://doi.org/10.1111/j.1365-2966.2007.12512.x
The peculiar horizontal branch morphology of the Galactic globular clusters NGC 6388 and NGC 6441: new insights from UV observations