Thick Disk Kinematics
Thick Disk Kinematics is a stellar kinematic framework that characterizes the distinct rotational and velocity dispersion properties of the Milky Way's thick disk population, differentiating it from the thin disk and halo components through its intermediate metallicity, older stellar age, and elevated vertical velocity dispersion.
127
Publications
10K
Citations
593
Authors
324
Institutions
Publications per year
2017–2026
25
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Osservatorio Astronomico di Padova
Padua, Italy
13 h-index
22 publications
1.6K citations
University of Cambridge
Cambridge, United Kingdom
12 h-index
21 publications
1.5K citations

University of Groningen
Groningen, The Netherlands
10 h-index
16 publications
824 citations

Johns Hopkins University
Baltimore, United States
10 h-index
13 publications
1K citations
National Astronomical Observatories
Beijing, China
9 h-index
40 publications
837 citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
25 publications
2.1K citations

Mount Stromlo Observatory
Canberra, Australia
9 h-index
15 publications
1.2K citations

University of Ljubljana
Ljubljana, Slovenia
8 h-index
8 publications
440 citations
1–8 of 324
ApJ · 35 publications · 3.1K citations
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AJ · 24 publications · 2.4K citations
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21 publications · 1.5K citations
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16 publications · 1.5K citations
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Repository · 4 publications · 62 citations
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