Reionization Feedback
Reionization Feedback is a theoretical astrophysical mechanism within cosmic structure formation that describes the suppression of gas accretion and star formation in low-mass halos due to the photoionizing radiation from early luminous sources during the epoch of reionization.
61
Publications
5.1K
Citations
157
Authors
106
Institutions
Publications per year
2017–2026
20
Parents
61
The morphology of H II regions during reionization
Matthew McQuinn, Adam Lidz, O. Zahn et al. · Monthly Notices of the Royal Astronomical Society · 2007 · 348 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 61
157
7
h-index
7
h-index
5
h-index
5
h-index
5
h-index
1–5 of 157
106
The University of Texas at Austin
Austin, United States
10 h-index
17 publications
1.7K citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
26 publications
3.9K citations
Scuola Normale Superiore
Pisa, Italy
7 h-index
11 publications
901 citations

University of Groningen
Groningen, The Netherlands
6 h-index
12 publications
557 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
6 h-index
18 publications
2.7K citations

The University of Melbourne
Melbourne, Australia
6 h-index
15 publications
724 citations
University of Sussex
Brighton, United Kingdom
6 h-index
8 publications
738 citations

Chosun University
Gwangju, South Korea
5 h-index
5 publications
496 citations
1–8 of 106
34 publications · 3.2K citations
25
h-index
ApJ · 15 publications · 1.2K citations
15
h-index
2 publications · 40 citations
2
h-index
2 publications · 78 citations
2
h-index
1 publications · 118 citations
1
h-index
1–5