Stellar Wind Accretion
Stellar Wind Accretion is a physical process in high-mass X-ray binary systems where a compact object captures and gravitationally binds matter from the supersonic outflow of its companion star’s atmosphere, distinguishing it from other accretion mechanisms by relying on the inherent dynamics of stellar wind rather than Roche-lobe overflow.
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Black Holes, Galaxy Formation, and the <i>M</i> <sub>BH</sub> - Relation
A. R. King · The Astrophysical Journal · 2003 · 808 citations · Full text
Natural Sciences, Astronomy, Physics +13
Black Hole Spin in X-Ray Binaries: Observational Consequences
The Astrophysical Journal · 1997 · 522 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
21 h-index
49 publications
6.1K citations
Goddard Space Flight Center
Greenbelt, United States
15 h-index
22 publications
1.4K citations

University of Leicester
Leicester, United Kingdom
14 h-index
37 publications
1.7K citations

Centre National de la Recherche Scientifique
Paris, France
11 h-index
16 publications
1.7K citations
University of Maryland, Baltimore County
Baltimore, United States
10 h-index
15 publications
681 citations
Technion – Israel Institute of Technology
Haifa, Israel
10 h-index
17 publications
414 citations
University of Geneva
Geneva, Switzerland
10 h-index
20 publications
456 citations
University of California, Berkeley
Berkeley, United States
10 h-index
12 publications
505 citations
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ApJ · 91 publications · 8.4K citations
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77 publications · 3K citations
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45 publications · 1.9K citations
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7 publications · 315 citations
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Repository · 7 publications · 324 citations
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