Barycentric Motion
Barycentric Motion is the orbital motion of two bodies in a gravitational system relative to their common center of mass, distinguished from absolute or geocentric motion by its reference frame being fixed at the system’s barycenter.
44
Publications
2.3K
Citations
113
Authors
89
Institutions
Publications per year
2017–2026
8
44
The LCES HIRES/Keck Precision Radial Velocity Exoplanet Survey
R. Paul Butler, Steven S. Vogt, Gregory Laughlin et al. · The Astronomical Journal · 2017 · 466 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 44
113
3
h-index
Laboratoire d’études spatiales et d’instrumentation en astrophysique, France
3 publications · 106 citations
3
h-index
2
h-index
European Space Research and Technology Centre, Netherlands
2 publications · 28 citations
2
h-index
2
h-index
1–5 of 113
89

Centre National de la Recherche Scientifique
Paris, France
6 h-index
12 publications
647 citations
Observatoire de la Côte d’Azur
Nice, France
4 h-index
7 publications
295 citations
University of Chile
Santiago, Chile
3 h-index
3 publications
546 citations
California Institute of Technology
Pasadena, United States
3 h-index
3 publications
113 citations
University of Missouri
Columbia, United States
3 h-index
3 publications
109 citations
University of California, Santa Cruz
Santa Cruz, United States
3 h-index
8 publications
2K citations
European Southern Observatory
Santiago, Chile
3 h-index
3 publications
172 citations
Université Paris Cité
Paris, France
3 h-index
3 publications
172 citations
1–8 of 89
AJ · 5 publications · 597 citations
5
h-index
5 publications · 266 citations
5
h-index
Repository · 3 publications · 73 citations
3
h-index
ApJ · 2 publications · 49 citations
2
h-index
PASP · 2 publications · 210 citations
2
h-index
1–5