Turbulent Fragmentation
Turbulent Fragmentation is a theoretical framework in star formation theory that explains the origin of stellar multiplicity and clustered star formation through the stochastic breakup of molecular cloud gas via supersonic turbulence, where density fluctuations induced by turbulent motions overcome local gravitational stability and lead to the hierarchical formation of gravitationally bound cores.
200
Publications
18.2K
Citations
433
Authors
255
Institutions
Publications per year
2017–2026
60
200
The Stellar Initial Mass Function from Turbulent Fragmentation
Paolo Padoan, Åke Nordlund · The Astrophysical Journal · 2002 · 1K citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 200
433
11
h-index
10
h-index
8
h-index
7
h-index
7
h-index
1–5 of 433
255
Cardiff University
Cardiff, United Kingdom
18 h-index
42 publications
2.2K citations

Centre National de la Recherche Scientifique
Paris, France
18 h-index
73 publications
6.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
17 h-index
31 publications
4.1K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
15 h-index
53 publications
6K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
15 h-index
23 publications
1.7K citations

University of Exeter
Exeter, United Kingdom
15 h-index
17 publications
3.6K citations

University of St Andrews
St Andrews, United Kingdom
13 h-index
18 publications
4.3K citations
CEA Paris-Saclay
Gif-sur-Yvette, France
12 h-index
47 publications
5.2K citations
1–8 of 255
ApJ · 51 publications · 6K citations
36
h-index
55 publications · 6.2K citations
35
h-index
23 publications · 2.2K citations
21
h-index
Repository · 6 publications · 226 citations
8
h-index
7 publications · 794 citations
7
h-index
1–5