Disk Dispersal
Disk Dispersal is a theoretical construct in astrophysics that describes the process by which circumstellar disks lose mass and dissipate over time due to mechanisms such as photoevaporation, accretion, and planet formation, thereby marking the transition from protoplanetary to debris disk phases.
104
Publications
8.7K
Citations
270
Authors
169
Institutions
Publications per year
2017–2026
37
Parents
104
Dynamics of Protoplanetary Disks
Annual Review of Astronomy and Astrophysics · 2011 · 494 citations · Full text
Natural Sciences, Astronomy, Physics +17
Dynamics of protoplanetary disks
Philip J. Armitage · 2016 · 289 citations
Natural Sciences, Astronomy, Physics +17
THE ROLE OF MULTIPLICITY IN DISK EVOLUTION AND PLANET FORMATION
Adam L. Kraus, Michael Ireland, Lynne A. Hillenbrand et al. · The Astrophysical Journal · 2011 · 280 citations · Full text
Natural Sciences, Astronomy, Physics +15
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270
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169

Centre National de la Recherche Scientifique
Paris, France
14 h-index
31 publications
2.8K citations
Leiden University
Leiden, The Netherlands
10 h-index
22 publications
1K citations
University of Cambridge
Cambridge, United Kingdom
10 h-index
16 publications
844 citations
Queen Mary University of London
London, United Kingdom
9 h-index
16 publications
919 citations
Excellence Cluster Universe
Garching, Germany
8 h-index
11 publications
824 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
8 h-index
17 publications
1.5K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
7 h-index
8 publications
483 citations

Search for Extraterrestrial Intelligence
Mountain View, United States
7 h-index
8 publications
585 citations
1–8 of 169
17 publications · 2.1K citations
17
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19 publications · 1.2K citations
16
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ApJ · 17 publications · 2.3K citations
15
h-index
9 publications · 457 citations
9
h-index
Repository · 6 publications · 183 citations
6
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1–5