Supernova-driven Gas
Supernova-Driven Gas is a dynamical state of interstellar gas characterized by bulk motion and thermal energization resulting directly from the mechanical energy input and shock propagation of nearby supernova explosions.
368
Publications
30.3K
Citations
1.1K
Authors
438
Institutions
Publications per year
2017–2026
59
Parents
368
Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows
Fabio Governato, Chris B. Brook, Lucio Mayer et al. · Nature · 2010 · 1K citations · Full text
Natural Sciences, Astronomy, Physics +15
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 368
1.1K
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Czech Academy of Sciences, Astronomical Institute, Czechia
7 publications · 948 citations
7
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1–5 of 1.1K
438
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
25 h-index
62 publications
5.8K citations
University of California, Berkeley
Berkeley, United States
22 h-index
43 publications
7.5K citations
Max Planck Institute for Astrophysics
Garching, Germany
20 h-index
52 publications
8.7K citations
University of California, Santa Cruz
Santa Cruz, United States
18 h-index
24 publications
3.4K citations
California Institute of Technology
Pasadena, United States
16 h-index
53 publications
12.1K citations
Heidelberg University
Heidelberg, Germany
15 h-index
37 publications
4.9K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
14 h-index
18 publications
1.3K citations
Princeton University
Princeton, United States
14 h-index
20 publications
1.7K citations
1–8 of 438
ApJ · 147 publications · 13.3K citations
63
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69 publications · 6.8K citations
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19 publications · 1K citations
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17 publications · 843 citations
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11 publications · 2.4K citations
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