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Cited article:

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SOME STARS ARE TOTALLY METAL: A NEW MECHANISM DRIVING DUST ACROSS STAR-FORMING CLOUDS, AND CONSEQUENCES FOR PLANETS, STARS, AND GALAXIES

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The puzzle of metallicity and multiple stellar populations in the globular clusters in Fornax

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Early disc accretion as the origin of abundance anomalies in globular clusters

N. Bastian, H. J. G. L. M. Lamers, S. E. de Mink, et al.
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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

Don A. VandenBerg, K. Brogaard, R. Leaman and L. Casagrande
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Constraining globular cluster formation through studies of young massive clusters – I. A lack of ongoing star formation within young clusters

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Pregalactic metal enrichment: The chemical signatures of the first stars

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Detailed abundance analysis from integrated high-dispersion spectroscopy: globular clusters in the Fornax dwarf spheroidal

S. S. Larsen, J. P. Brodie and J. Strader
Astronomy & Astrophysics 546 A53 (2012)
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FORMATION OF METAL-POOR GLOBULAR CLUSTERS IN Lyα EMITTING GALAXIES IN THE EARLY UNIVERSE

Bruce G. Elmegreen, Sangeeta Malhotra and James Rhoads
The Astrophysical Journal 757 (1) 9 (2012)
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