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Cited article:

Apparent high metallicity in 3–4 keV galaxy clusters: the inverse iron-bias in action in the case of the merging cluster Abell 2028

F. Gastaldello, S. Ettori, I. Balestra, et al.
Astronomy & Astrophysics 522 A34 (2010)
https://doi.org/10.1051/0004-6361/201014279

Morphology and evolution of simulated and optical clusters: a comparative analysis

N. Rahman, J. Krywult, P. M. Motl, P. Flin and S. F. Shandarin
Monthly Notices of the Royal Astronomical Society 367 (2) 838 (2006)
https://doi.org/10.1111/j.1365-2966.2005.10014.x

Temperature and Heavy‐Element Abundance Profiles of Cool Clusters of Galaxies fromASCA

A. Finoguenov, M. Arnaud and L. P. David
The Astrophysical Journal 555 (1) 191 (2001)
https://doi.org/10.1086/321457

Optical Luminosities and Mass‐to‐Light Ratios of Nearby Galaxy Clusters

Marisa Girardi, Stefano Borgani, Giuliano Giuricin, Fabio Mardirossian and Marino Mezzetti
The Astrophysical Journal 530 (1) 62 (2000)
https://doi.org/10.1086/308342

An X‐Ray and Optical Study of Matter Distribution in the Galaxy Cluster A2319

D. Trevese, G. Cirimele and M. De Simone
The Astrophysical Journal 530 (2) 680 (2000)
https://doi.org/10.1086/308381