Binary Orbital Modulation
Binary Orbital Modulation is a periodic variation in the observed X-ray emission from a compact object in a binary system, arising from the orbital motion that modulates the line-of-sight to the X-ray source through Doppler shifts, eclipse effects, or changes in accretion geometry.
189
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8.5K
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799
Authors
326
Institutions
Publications per year
2017–2026
40
Parents
189
Variable Very-High-Energy Gamma-Ray Emission from the Microquasar LS I +61 303
J. Albert, E. Aliu, H. Anderhub et al. · Science · 2006 · 413 citations · Full text
Natural Sciences, Astronomy, Physics +13
Discovery of a Second Millisecond Accreting Pulsar: XTE J1751−305
C. B. Markwardt, J. H. Swank, Tod E. Strohmayer et al. · The Astrophysical Journal · 2002 · 192 citations · Full text
Natural Sciences, Astronomy, Physics +14
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326

University of Amsterdam
Amsterdam, The Netherlands
14 h-index
23 publications
1.2K citations
Goddard Space Flight Center
Greenbelt, United States
12 h-index
24 publications
1.3K citations
Massachusetts Institute of Technology
Cambridge, United States
11 h-index
14 publications
684 citations
Universitat de Barcelona
Barcelona, Spain
9 h-index
26 publications
698 citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
9 h-index
14 publications
458 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
13 publications
688 citations
KU Leuven
Leuven, Belgium
8 h-index
30 publications
1.5K citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
39 publications
8.2K citations
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ApJ · 50 publications · 3K citations
29
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48 publications · 1.9K citations
26
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32 publications · 1.4K citations
22
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9 publications · 315 citations
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AJ · 6 publications · 182 citations
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