Orbital Separation Distribution
Orbital Separation Distribution is a statistical construct in astrophysics that characterizes the frequency distribution of projected or physical distances between components in binary star systems, distinguishing it from other binary properties by quantifying the likelihood of formation or survival at specific separations.
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8.4K
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628
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312
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2017–2026
41
Parents
130
New companions to nearby low-mass stars
Esther Jódar, A. Pérez‐Garrido, A. Díaz‐Sánchez et al. · Monthly Notices of the Royal Astronomical Society · 2012 · 252 citations
Natural Sciences, Astronomy, Physics +14
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California Institute of Technology
Pasadena, United States
13 h-index
18 publications
2.8K citations

Centre National de la Recherche Scientifique
Paris, France
11 h-index
191 publications
23.3K citations
Leiden University
Leiden, The Netherlands
9 h-index
12 publications
816 citations
University of Arizona
Tucson, United States
9 h-index
14 publications
1.1K citations

Space Telescope Science Institute
Baltimore, United States
9 h-index
12 publications
1.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
8 h-index
50 publications
5.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
8 h-index
13 publications
898 citations
University of Michigan
Ann Arbor, United States
7 h-index
8 publications
443 citations
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ApJ · 32 publications · 2.4K citations
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26 publications · 1.9K citations
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AJ · 21 publications · 1.7K citations
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10 publications · 644 citations
10
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5 publications · 357 citations
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