Feedback-driven Turbulence
Feedback-Driven Turbulence is a type of interstellar turbulence sustained by the mechanical and radiative energy input from massive stars, supernovae, and stellar winds, which inject kinetic energy into star-forming regions and regulate gas dynamics, star formation efficiency, and the structural evolution of molecular clouds.
33
Publications
2.2K
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106
Authors
98
Institutions
Publications per year
2017–2026
16
33
Gravity‐driven Turbulence in Galactic Disks
The Astrophysical Journal · 2002 · 166 citations · Full text
Natural Sciences, Astronomy, Physics +16
Mutual influence of supernovae and molecular clouds
Olivier Iffrig, P. Hennebelle · Astronomy and Astrophysics · 2015 · 125 citations · Full text
Natural Sciences, Astronomy, Physics +14
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98

Australian National University
Canberra, Australia
6 h-index
11 publications
741 citations

Centre National de la Recherche Scientifique
Paris, France
4 h-index
10 publications
630 citations
University of California, Santa Cruz
Santa Cruz, United States
3 h-index
4 publications
365 citations
Chalmers University of Technology
Gothenburg, Sweden
3 h-index
3 publications
160 citations
Astrophysique, Instrumentation et Modélisation
Gif-sur-Yvette, France
3 h-index
7 publications
442 citations
CEA Paris-Saclay
Gif-sur-Yvette, France
3 h-index
7 publications
442 citations
ASTRO-3D
Australind, Australia
3 h-index
7 publications
427 citations
Flatiron Health (United States)
New York, United States
3 h-index
4 publications
474 citations
1–8 of 98
19 publications · 1.3K citations
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ApJ · 5 publications · 504 citations
5
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1 publications · 86 citations
1
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1 publications · 82 citations
1
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1 publications · 48 citations
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