Galaxy Size Evolution
Galaxy Size Evolution is a theoretical framework in astrophysics that characterizes the temporal changes in the physical scale of galaxies as a function of cosmic time, distinguishing itself from other galactic evolution models by focusing specifically on the growth and structural expansion mechanisms driven by merger histories, accretion processes, and internal dynamical feedback.
313
Publications
31K
Citations
926
Authors
389
Institutions
Publications per year
2017–2026
90
Parents
313
THE GROWTH OF MASSIVE GALAXIES SINCE<i>z</i>= 2
Pieter van Dokkum, Katherine E. Whitaker, Gabriel Brammer et al. · The Astrophysical Journal · 2010 · 816 citations · Full text
Natural Sciences, Astronomy, Physics +15
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389
Leiden University
Leiden, The Netherlands
31 h-index
71 publications
14.5K citations
California Institute of Technology
Pasadena, United States
24 h-index
46 publications
6.7K citations

Space Telescope Science Institute
Baltimore, United States
23 h-index
63 publications
7K citations

Centre National de la Recherche Scientifique
Paris, France
23 h-index
96 publications
6.9K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
22 h-index
49 publications
9.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
22 h-index
39 publications
7.2K citations
Max Planck Institute for Astrophysics
Garching, Germany
22 h-index
29 publications
7.3K citations
Yale University
New Haven, United States
21 h-index
47 publications
13.8K citations
1–8 of 389
ApJ · 89 publications · 12.3K citations
57
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92 publications · 8.8K citations
46
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23 publications · 1.2K citations
18
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14 publications · 1.4K citations
15
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7 publications · 440 citations
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