Protoplanetary Disk Viscosity is a physical property representing the internal friction within a protoplanetary disk that governs the rate of angular momentum transport and mass accretion, distinguishing it from other disk dynamics by its direct influence on planetary migration and disk evolution.
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195
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2017–2026
73
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Publications
167
Flows of gas through a protoplanetary gap
Simón Casassus, G. van der Plas, Sebastián Pérez et al. · Nature · 2013 · 386 citations · Full text
The evolution of the water distribution in a viscous protoplanetary disk
F. J. Ciesla, J. N. Cuzzi · Icarus · 2005 · 351 citations · Full text
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1–5 of 251
Institutions
195
Max Planck Institute for Astronomy
Heidelberg, Germany
20 h-index
37 publications
2.2K citations
Centre National de la Recherche Scientifique
Paris, France
18 h-index
37 publications
3.2K citations
University of Cambridge
Cambridge, United Kingdom
16 h-index
29 publications
1.2K citations
Queen Mary University of London
London, United Kingdom
10 h-index
13 publications
1.5K citations
Observatoire de la Côte d’Azur
Nice, France
10 h-index
16 publications
1.7K citations
Leiden University
Leiden, The Netherlands
9 h-index
20 publications
1.5K citations
Université Côte d'Azur
Nice, France
8 h-index
14 publications
1.2K citations
Heidelberg University
Heidelberg, Germany
7 h-index
8 publications
528 citations
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- The Astrophysical Journal
ApJ · 59 publications · 5.1K citations
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- Monthly Notices of the Royal Astronomical Society
35 publications · 1.8K citations
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- Astronomy and Astrophysics
24 publications · 1.7K citations
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- Springer Link (Chiba Institute of Technology)
Repository · 10 publications · 536 citations
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- The Astrophysical Journal Letters
8 publications · 641 citations
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