Moving Group Analysis
Moving Group Analysis is a methodological framework in astrophysics that identifies and characterizes co-moving associations of stars sharing common kinematic and spatial trajectories within the Galaxy, distinguished from other stellar population analyses by its focus on velocity coherence as evidence of shared dynamical origin.
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6.5K
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243
Authors
139
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2017–2026
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A [ITAL]Hipparcos[/ITAL] Census of the Nearby OB Associations
P. T. de Zeeuw, R. Hoogerwerf, J. H. J. de Bruijne et al. · The Astronomical Journal · 1999 · 1.3K citations · Full text
Natural Sciences, Astronomy, Physics +17
B. Zuckerman, Inseok Song, M. S. Bessell · The Astrophysical Journal · 2004 · 224 citations
Natural Sciences, Astronomy, Physics +12
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Max Planck Institute for Astronomy
Heidelberg, Germany
9 h-index
14 publications
1.4K citations
Universidad Complutense de Madrid
Madrid, Spain
8 h-index
19 publications
1.3K citations

Australian National University
Canberra, Australia
7 h-index
22 publications
1.1K citations

American Museum of Natural History
New York, United States
6 h-index
12 publications
891 citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
10 publications
367 citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
5 h-index
5 publications
155 citations
Centro de Astrobiología
Torrejón de Ardoz, Spain
5 h-index
11 publications
412 citations

Observatoire astronomique de Strasbourg
Strasbourg, France
5 h-index
10 publications
355 citations
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19 publications · 1.5K citations
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15 publications · 907 citations
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ApJ · 13 publications · 1.4K citations
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AJ · 12 publications · 2K citations
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Repository · 2 publications · 39 citations
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