Accretion Disk Polarization
Accretion Disk Polarization is a theoretical model in X-ray polarimetry that characterizes the linear polarization of X-ray emission arising from relativistic accretion disks around compact objects due to the preferential scattering of photons in strong gravitational and magnetic fields.
123
Publications
6.3K
Citations
423
Authors
285
Institutions
Publications per year
2017–2026
37
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1–5 of 123
423
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Czech Academy of Sciences, Astronomical Institute, Czechia
16 publications · 539 citations
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1–5 of 423
285

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
17 h-index
54 publications
2.1K citations
Roma Tre University
Rome, Italy
16 h-index
49 publications
1.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
52 publications
3.1K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
33 publications
1.3K citations

Stockholm University
Stockholm, Sweden
12 h-index
14 publications
505 citations

Washington University in St. Louis
St Louis, United States
12 h-index
29 publications
1K citations

University of Turku
Turku, Finland
12 h-index
47 publications
1.5K citations

KTH Royal Institute of Technology
Stockholm, Sweden
12 h-index
20 publications
835 citations
1–8 of 285
ApJ · 47 publications · 2.7K citations
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32 publications · 1.7K citations
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12 publications · 441 citations
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5 publications · 189 citations
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Repository · 4 publications · 466 citations
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