Inner Disk Structure
Inner Disk Structure is a theoretical construct in astrophysics that characterizes the physical and dynamical organization of matter in the region of an accretion disk closest to the central compact object, distinguished by relativistic effects, intense radiation fields, and viscosity-driven transport processes.
726
Publications
48.4K
Citations
2.5K
Authors
709
Institutions
Publications per year
2017–2026
174
Parents
726
Hyperaccreting Black Holes and Gamma‐Ray Bursts
Robert Popham, S. E. Woosley, Chris L. Fryer · The Astrophysical Journal · 1999 · 818 citations · Full text
Natural Sciences, Astronomy, Physics +16
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709
California Institute of Technology
Pasadena, United States
59 h-index
272 publications
35K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
54 h-index
192 publications
23.5K citations

Centre National de la Recherche Scientifique
Paris, France
53 h-index
341 publications
29.5K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
42 h-index
207 publications
15.2K citations
University of Michigan
Ann Arbor, United States
41 h-index
143 publications
10.6K citations
Jet Propulsion Laboratory
Pasadena, United States
39 h-index
114 publications
8.6K citations
University of Cambridge
Cambridge, United Kingdom
38 h-index
96 publications
7.3K citations
Leiden University
Leiden, The Netherlands
38 h-index
129 publications
10K citations
1–8 of 709
ApJ · 303 publications · 22.3K citations
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130 publications · 7.4K citations
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AJ · 45 publications · 3.7K citations
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32 publications · 2.6K citations
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35 publications · 1.8K citations
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