Disk Instability Model
The Disk Instability Model is a theoretical framework in astrophysics that explains the episodic outbursts in X-ray binaries through thermal-viscous instabilities in the accretion disk, distinguishing it from steady accretion models by attributing variability to opacity-driven transitions in the disk’s ionization state.
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Centre National de la Recherche Scientifique
Paris, France
25 h-index
81 publications
5.3K citations
Institut d'Astrophysique de Paris
Paris, France
18 h-index
24 publications
2K citations

Sorbonne Université
Paris, France
16 h-index
23 publications
1K citations

University of Leicester
Leicester, United Kingdom
14 h-index
22 publications
1.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
14 h-index
20 publications
2K citations
Goddard Space Flight Center
Greenbelt, United States
13 h-index
20 publications
1.1K citations

Carnegie Institution for Science
Washington, United States
13 h-index
13 publications
1.8K citations
Carnegie Observatories
Pasadena, United States
13 h-index
13 publications
1.8K citations
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ApJ · 97 publications · 9K citations
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