Accretion Histories
Accretion History is a theoretical construct in astrophysics that denotes the chronological sequence and characteristics of mergers and mass incorporations through which a galaxy, particularly its halo, has grown over time by capturing smaller satellite systems and globular clusters.
175
Publications
22.7K
Citations
530
Authors
326
Institutions
Publications per year
2017–2026
58
175
Concentrations of Dark Halos from Their Assembly Histories
Risa H. Wechsler, James S. Bullock, Joel R. Primack et al. · The Astrophysical Journal · 2002 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 175
530
6
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Kavli Institute for Particle Astrophysics and Cosmology, United States
6 publications · 4.4K citations
6
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Center for Astrophysics Harvard & Smithsonian, United States
6 publications · 721 citations
6
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5
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1–5 of 530
326

Centre National de la Recherche Scientifique
Paris, France
17 h-index
48 publications
3.7K citations
Max Planck Institute for Astrophysics
Garching, Germany
16 h-index
31 publications
9.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
14 h-index
20 publications
1.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
11 h-index
17 publications
1.1K citations

Durham University
Durham, United Kingdom
10 h-index
26 publications
5.5K citations
Kavli Institute for Particle Astrophysics and Cosmology
Menlo Park, United States
9 h-index
13 publications
6.1K citations
University of California, Santa Cruz
Santa Cruz, United States
9 h-index
11 publications
5.8K citations
Max Planck Society
Munich, Germany
9 h-index
12 publications
5.4K citations
1–8 of 326
60 publications · 6.8K citations
36
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ApJ · 36 publications · 8.8K citations
31
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19 publications · 1.1K citations
17
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4 publications · 1.3K citations
4
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3 publications · 325 citations
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