Protoplanetary Disk Evolution
Protoplanetary Disk Evolution is the process by which a rotating circumstellar disk of gas and dust undergoes structural, thermal, and compositional changes over time due to gravitational, radiative, and hydrodynamic interactions, ultimately governing the conditions for planetary formation and early system architecture.
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Protoplanetary Disks and Their Evolution
Annual Review of Astronomy and Astrophysics · 2011 · 1.3K citations · Full text
Natural Sciences, Astronomy, Physics +16
M. C. Wyatt · Annual Review of Astronomy and Astrophysics · 2008 · 960 citations
Natural Sciences, Astronomy, Physics +17
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Max Planck Institute for Astronomy
Heidelberg, Germany
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225 publications
21.1K citations

Centre National de la Recherche Scientifique
Paris, France
54 h-index
427 publications
30.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
52 h-index
165 publications
19.4K citations
Leiden University
Leiden, The Netherlands
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189 publications
19.5K citations
University of Cambridge
Cambridge, United Kingdom
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115 publications
9.1K citations
California Institute of Technology
Pasadena, United States
37 h-index
69 publications
10.5K citations
European Southern Observatory
Garching bei München, Germany
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99 publications
9.4K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
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ApJ · 271 publications · 23.4K citations
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Repository · 39 publications · 1.8K citations
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