Inner Disk Holes
Inner Disk Holes is a structural feature in protoplanetary disks characterized by a depleted or absent region of dust and gas in the central few astronomical units, distinguishing it from continuous disk models by indicating potential planet formation or dynamical clearing processes.
74
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7.3K
Citations
353
Authors
187
Institutions
Publications per year
2017–2026
7
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RESOLVED IMAGES OF LARGE CAVITIES IN PROTOPLANETARY TRANSITION DISKS
The Astrophysical Journal · 2011 · 654 citations · Full text
Natural Sciences, Astronomy, Physics +13
Circumstellar Disks in the Orion Nebula Cluster
Lynne A. Hillenbrand, S. E. Strom, Nuria Calvet et al. · The Astronomical Journal · 1998 · 266 citations · Full text
Natural Sciences, Astronomy, Physics +15
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Center for Astrophysics Harvard & Smithsonian, United States
4 publications · 477 citations
4
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4
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1–5 of 353
187
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
43 publications
7.1K citations
Leiden University
Leiden, The Netherlands
11 h-index
20 publications
2.4K citations
University of Michigan
Ann Arbor, United States
10 h-index
16 publications
2.3K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
10 h-index
27 publications
2K citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
18 publications
1.7K citations
Jet Propulsion Laboratory
Pasadena, United States
9 h-index
13 publications
1.3K citations
University of Arizona
Tucson, United States
8 h-index
14 publications
955 citations
California Institute of Technology
Pasadena, United States
8 h-index
13 publications
2.5K citations
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ApJ · 35 publications · 4.3K citations
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10 publications · 448 citations
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4 publications · 445 citations
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AJ · 3 publications · 701 citations
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3 publications · 182 citations
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