Host Galaxy Coevolution
Host Galaxy Coevolution is a theoretical framework in astrophysics that describes the mutual development and dynamical interaction between supermassive black holes and their host galaxies over cosmic time, driven by processes such as mergers, feedback mechanisms, and star formation regulation.
44
Publications
10K
Citations
227
Authors
160
Institutions
Publications per year
2017–2026
21
Variants
Black Hole-galaxy Coevolution
Parents
44
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
2013 · 1.5K citations
Natural Sciences, Astronomy, Physics +14
A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
2003 · 622 citations
Natural Sciences, Astronomy, Physics +15
1–5 of 44
227
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3
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1–5 of 227
160
Princeton University
Princeton, United States
7 h-index
10 publications
558 citations

Pennsylvania State University
State College, United States
5 h-index
12 publications
643 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
9 publications
1.2K citations

Durham University
Durham, United Kingdom
5 h-index
5 publications
495 citations
Institute of Astronomy and Astrophysics, Academia Sinica
Taipei, Taiwan
4 h-index
4 publications
111 citations
University of Southampton
Southampton, United Kingdom
4 h-index
7 publications
263 citations

Kyoto University
Kyoto, Japan
4 h-index
7 publications
143 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
9 publications
2.2K citations
1–8 of 160
ApJ · 19 publications · 2.1K citations
17
h-index
9 publications · 662 citations
9
h-index
3 publications · 193 citations
3
h-index
2 publications · 36 citations
2
h-index
2 publications · 339 citations
2
h-index
1–5