Streaming Instability
Streaming Instability is a hydrodynamic instability in protoplanetary disks that constitutes a theoretical mechanism wherein solid particles and gas interact through drag forces, leading to the spontaneous concentration of solids into dense clumps capable of undergoing gravitational collapse to form planetesimals.
245
Publications
18.5K
Citations
377
Authors
245
Institutions
Publications per year
2017–2026
110
245
Streaming Instabilities in Protoplanetary Disks
The Astrophysical Journal · 2005 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +15
Streaming Instabilities in Protoplanetary Disks
2004 · 524 citations
Natural Sciences, Astronomy, Physics +15
1–5 of 245
377
16
h-index
10
h-index
8
h-index
Joint Institute for Laboratory Astrophysics, United States
8 publications · 772 citations
8
h-index
7
h-index
1–5 of 377
245

Lund University
Lund, Sweden
23 h-index
60 publications
5.8K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
16 h-index
33 publications
2.3K citations
University of Arizona
Tucson, United States
13 h-index
20 publications
2.1K citations

Centre National de la Recherche Scientifique
Paris, France
13 h-index
33 publications
1.4K citations
Princeton University
Princeton, United States
10 h-index
16 publications
4.7K citations

Joint Institute for Laboratory Astrophysics
Boulder, United States
9 h-index
15 publications
1.8K citations

Southwest Research Institute
San Antonio, United States
9 h-index
11 publications
1.1K citations
Los Alamos National Laboratory
Los Alamos, United States
8 h-index
14 publications
378 citations
1–8 of 245
ApJ · 58 publications · 6.3K citations
37
h-index
39 publications · 3.6K citations
30
h-index
38 publications · 1.8K citations
24
h-index
Repository · 14 publications · 1.1K citations
12
h-index
10 publications · 785 citations
10
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1–5