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Cited article:

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Confirmation of a metallicity spread amongst first population stars in globular clusters

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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

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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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The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters

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THEHUBBLE SPACE TELESCOPEUV LEGACY SURVEY OF GALACTIC GLOBULAR CLUSTERS. III. A QUINTUPLE STELLAR POPULATION IN NGC 2808

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Theoretical evolutionary framework for low-mass stars in massive star clusters

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Evolutionary stellar population synthesis with MILES – II. Scaled-solar and α-enhanced models

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The Hubble Space Telescope UV Legacy Survey of galactic globular clusters – II. The seven stellar populations of NGC 7089 (M2)⋆

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Helium enhanced stars and multiple populations along the horizontal branch of NGC 2808: direct spectroscopic measurements★

A. F. Marino, A. P. Milone, N. Przybilla, et al.
Monthly Notices of the Royal Astronomical Society 437 (2) 1609 (2014)
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ISOCHRONES FOR OLD (>5 GYR) STARS AND STELLAR POPULATIONS. I. MODELS FOR –2.4 ⩽ [Fe/H] ⩽+0.6, 0.25 ⩽Y⩽ 0.33, AND –0.4 ⩽ [α/Fe] ⩽+0.4

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THE CARINA PROJECT. VII. TOWARD THE BREAKING OF THE AGE-METALLICITY DEGENERACY OF RED GIANT BRANCH STARS USING THECU, B, IINDEX

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The M 4 Core Project with HST – II. Multiple stellar populations at the bottom of the main sequence

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On the missing second generation AGB stars in NGC 6752

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THE AGES OF 55 GLOBULAR CLUSTERS AS DETERMINED USING AN IMPROVED $\Delta V^{\rm HB}_{\rm TO}$ METHOD ALONG WITH COLOR-MAGNITUDE DIAGRAM CONSTRAINTS, AND THEIR IMPLICATIONS FOR BROADER ISSUES

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The Astrophysical Journal 775 (2) 134 (2013)
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