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Globular Clusters and Galaxy Formation in Clusters of Galaxies
1984Taken at face value globular cluster counts indicate that: (1) Most elliptical galaxies in rich clusters were not formed by merging spirals and (2) central galaxies in rich clusters were already very special at the time when they were forming globular clusters.
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Galaxy Environment and Clusters of Galaxies
1994The galaxy population of clusters of galaxies is clearly different from the “field” population. While some of the static parameters, morphology for instance, are quite likely defined at formation, others, HI content, are strongly modified during the cluster lifetime due to the interaction of the objects with their environment.
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The First Galaxies and Galaxy Clusters
2009Obvious targets for Extremely Large Telescopes are high-redshift galaxies and galaxy (proto-)clusters. However, due to the extremely small field-of-view of such telescopes, finding such objects, notably the rarer proto-clusters, is best be done using other facilities.
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ACM SIGGRAPH 99 Electronic art and animation catalog, 1999
John Dubinski +3 more
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John Dubinski +3 more
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Spectroscopic confirmation of a mature galaxy cluster at a redshift of 2
Nature, 2020Adam Mantz, R E A Canning, A L King
exaly
A single population of red globular clusters around the massive compact galaxy NGC 1277
Nature, 2018Ryan Leaman +2 more
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A massive core for a cluster of galaxies at a redshift of 4.3
Nature, 2018Allison L. Strom +2 more
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A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies
Nature, 2012Michael McDonald +2 more
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TheThreeHundred project: backsplash galaxies in simulations of clusters
Monthly Notices of the Royal Astronomical Society, 2020Gustavo Yepes, Roan Haggar, Weiguang Cui
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