Dynamical Parallax
Dynamical Parallax is a method in astrophysics that determines the distance to a binary star system by combining observational measurements of its orbital parameters and apparent brightness with Keplerian dynamics and mass-luminosity relations to infer parallax indirectly.
57
Publications
2.9K
Citations
169
Authors
96
Institutions
Publications per year
2017–2026
7
Parents
57
OGLE‐2003‐BLG‐262: Finite‐Source Effects from a Point‐Mass Lens
The Astrophysical Journal · 2004 · 412 citations · Full text
Natural Sciences, Astronomy, Physics +12
SPECKLE INTERFEROMETRY AND ORBITS OF “FAST” VISUAL BINARIES
The Astronomical Journal · 2012 · 233 citations · Full text
Natural Sciences, Astronomy, Physics +15
2 Speckle interferometry and orbits of “fast ” visual binaries
Andreï Tokovinin · 2016 · 223 citations
Natural Sciences, Astronomy, Physics +15
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96
Cerro Tololo Inter-American Observatory
La Serena, Chile
6 h-index
11 publications
771 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
7 publications
472 citations
The Ohio State University
Columbus, United States
4 h-index
8 publications
825 citations
United States Naval Observatory
Flagstaff, United States
3 h-index
5 publications
846 citations
Astronomical Observatory
Belgrade, Serbia
3 h-index
6 publications
100 citations
Institute of Astronomy
Moscow, Russia
2 h-index
9 publications
106 citations

Brera Astronomical Observatory
Milan, Italy
2 h-index
3 publications
57 citations
Universidade de Santiago de Compostela
Santiago de Compostela, Spain
2 h-index
4 publications
72 citations
1–8 of 96
ApJ · 16 publications · 1.5K citations
14
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AJ · 9 publications · 245 citations
9
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6 publications · 211 citations
6
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PASP · 4 publications · 88 citations
4
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4 publications · 170 citations
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