Driven Turbulence
Driven Turbulence is a type of turbulence in star-forming regions characterized by the sustained injection of kinetic energy through external or internal mechanisms, such as stellar feedback or large-scale gravitational flows, that actively maintain turbulent motions against dissipative processes.
115
Publications
7.5K
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343
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223
Institutions
Publications per year
2017–2026
22
Variants
Forced Turbulence
115
Protostellar Turbulence Driven by Collimated Outflows
The Astrophysical Journal · 2007 · 257 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 115
343
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Joint Institute for Laboratory Astrophysics, United States
3 publications · 301 citations
3
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1–5 of 343
223

Centre National de la Recherche Scientifique
Paris, France
7 h-index
20 publications
1.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
7 h-index
12 publications
1.2K citations
The University of Texas at Austin
Austin, United States
7 h-index
27 publications
531 citations
University of Wisconsin–Madison
Madison, United States
5 h-index
7 publications
589 citations
Heidelberg University
Heidelberg, Germany
5 h-index
8 publications
1.9K citations
University of California, Berkeley
Berkeley, United States
5 h-index
12 publications
686 citations
University of California San Diego
San Diego, United States
5 h-index
14 publications
662 citations
Technische Universität Berlin
Berlin, Germany
5 h-index
13 publications
1.2K citations
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ApJ · 27 publications · 2.1K citations
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13 publications · 826 citations
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12 publications · 1.2K citations
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10 publications · 564 citations
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PRL · 8 publications · 722 citations
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