Ionizing Stellar Sources is a theoretical construct in astrophysics denoting massive, hot stars whose spectral energy distribution predominantly emits photons with sufficient energy to ionize hydrogen atoms in surrounding interstellar medium, thereby initiating and sustaining H II regions.
436
Publications
24.7K
Citations
1.5K
Authors
509
Institutions
Publications per year
2017–2026
57
Variants
Ionizing Stars
Parents
Publications
436
Heating and Ionization of HI Regions
A. Dalgarno, Richard McCray · Annual Review of Astronomy and Astrophysics · 1972 · 809 citations
Natural Sciences, Physics, Heating +10
1–5 of 436
Authors
1.5K
- WM
9
h-index
- SC
6
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- PG
6
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- JC
6
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- DR
5
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1–5 of 1.5K
Institutions
509
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
26 h-index
49 publications
3K citations
Centre National de la Recherche Scientifique
Paris, France
26 h-index
101 publications
8.2K citations
Space Telescope Science Institute
Baltimore, United States
21 h-index
35 publications
4.6K citations
California Institute of Technology
Pasadena, United States
20 h-index
56 publications
7.4K citations
University of Arizona
Tucson, United States
18 h-index
48 publications
6.3K citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
15 h-index
53 publications
1.8K citations
Arcetri Astrophysical Observatory
Florence, Italy
15 h-index
29 publications
2.2K citations
University of California, Berkeley
Berkeley, United States
14 h-index
25 publications
1.5K citations
1–8 of 509
Venues
- The Astrophysical Journal
ApJ · 180 publications · 10K citations
57
h-index
- Monthly Notices of the Royal Astronomical Society
89 publications · 6.2K citations
46
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- Astronomy and Astrophysics
43 publications · 2.3K citations
26
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- The Astronomical Journal
AJ · 21 publications · 1.1K citations
15
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- Nature
9 publications · 389 citations
9
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1–5