Galaxy Morphology Evolution
Galaxy Morphology Evolution is a theoretical construct in astrophysics that characterizes the transformation over cosmic time in the structural forms of galaxies, such as their shape, size, and component distribution, as driven by internal processes and external interactions within the broader framework of galaxy formation and evolution.
643
Publications
59.1K
Citations
2.6K
Authors
647
Institutions
Publications per year
2017–2026
185
643
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
2013 · 1.5K citations
Natural Sciences, Astronomy, Physics +14
1–5 of 643
2.6K
17
h-index
15
h-index
13
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12
h-index
12
h-index
1–5 of 2.6K
647

Centre National de la Recherche Scientifique
Paris, France
44 h-index
275 publications
24.8K citations

Space Telescope Science Institute
Baltimore, United States
39 h-index
108 publications
13.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
36 h-index
100 publications
23K citations
California Institute of Technology
Pasadena, United States
35 h-index
102 publications
13.7K citations
European Southern Observatory
Garching bei München, Germany
31 h-index
63 publications
4.5K citations

Johns Hopkins University
Baltimore, United States
29 h-index
57 publications
10.3K citations
Laboratoire d’Astrophysique de Marseille
Marseille, France
28 h-index
92 publications
11.2K citations
University of Oxford
Oxford, United Kingdom
27 h-index
60 publications
7.1K citations
1–8 of 647
ApJ · 133 publications · 15.7K citations
60
h-index
180 publications · 13.6K citations
59
h-index
89 publications · 6.4K citations
40
h-index
AJ · 33 publications · 1.8K citations
23
h-index
Repository · 14 publications · 711 citations
13
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1–5