Disk Surface Density Profiles
Disk Surface Density Profile is a mathematical representation of the spatial distribution of mass per unit area across a circumstellar disk, distinguishing itself by quantifying how surface density varies radially from the central star, thereby governing the dynamics of planetary migration.
152
Publications
14.4K
Citations
371
Authors
240
Institutions
Publications per year
2017–2026
31
Variants
Disk Surface Density Profile
152
1–5 of 152
371
7
h-index
7
h-index
6
h-index
5
h-index
5
h-index
1–5 of 371
240

Centre National de la Recherche Scientifique
Paris, France
15 h-index
37 publications
3.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
13 h-index
31 publications
2.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
12 h-index
21 publications
2.3K citations
Leiden University
Leiden, The Netherlands
11 h-index
16 publications
2K citations
California Institute of Technology
Pasadena, United States
10 h-index
17 publications
3K citations

Observatoire astronomique de Strasbourg
Strasbourg, France
8 h-index
13 publications
1.2K citations
University of California, Berkeley
Berkeley, United States
7 h-index
11 publications
1.6K citations
University of California, Santa Cruz
Santa Cruz, United States
7 h-index
13 publications
794 citations
1–8 of 240
ApJ · 71 publications · 7.3K citations
43
h-index
22 publications · 2.3K citations
19
h-index
12 publications · 1.4K citations
12
h-index
4 publications · 223 citations
4
h-index
AJ · 4 publications · 149 citations
4
h-index
1–5