Massive Galaxy Clusters
Massive Galaxy Clusters is a cosmological construct denoting the most gravitationally bound and massive assemblies of galaxies, dark matter, and hot intracluster gas, distinguished by their high X-ray luminosity, strong gravitational lensing effects, and role as probes of large-scale structure formation in the universe.
2.3K
Publications
176.4K
Citations
6K
Authors
1.1K
Institutions
Publications per year
2017–2026
652
Parents
2.3K
Galaxy formation through hierarchical clustering
Simon D. M. White, Carlos S. Frenk · The Astrophysical Journal · 1991 · 2.3K citations · Full text
Natural Sciences, Astronomy, Physics +16
Cluster evolution as a diagnostic for Ω
V. R. Eke, Shaun Cole, Carlos S. Frenk · Monthly Notices of the Royal Astronomical Society · 1996 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 2.3K
6K
48
h-index
43
h-index
35
h-index
34
h-index
33
h-index
1–5 of 6K
1.1K
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
83 h-index
505 publications
52.3K citations
California Institute of Technology
Pasadena, United States
81 h-index
484 publications
49K citations

Durham University
Durham, United Kingdom
78 h-index
357 publications
44K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
76 h-index
554 publications
34.9K citations

Centre National de la Recherche Scientifique
Paris, France
75 h-index
943 publications
86.7K citations
Leiden University
Leiden, The Netherlands
73 h-index
362 publications
26.5K citations
Max Planck Institute for Astrophysics
Garching, Germany
71 h-index
237 publications
36.5K citations

Space Telescope Science Institute
Baltimore, United States
70 h-index
397 publications
56.5K citations
1–8 of 1.1K
ApJ · 644 publications · 56.1K citations
126
h-index
701 publications · 54.5K citations
116
h-index
275 publications · 16.2K citations
69
h-index
AJ · 69 publications · 6.2K citations
41
h-index
73 publications · 4.5K citations
40
h-index
1–5