Disk Stellar Populations
Disk Stellar Populations is a stellar population category comprising stars that reside in the disk component of a galaxy, distinguished by their spatial distribution, relatively high metallicity, and kinematic properties associated with rotational support.
417
Publications
36.1K
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1.2K
Authors
469
Institutions
Publications per year
2017–2026
75
Parents
417
Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation
The Astrophysical Journal · 2001 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +16
Disk Frequencies and Lifetimes in Young Clusters
The Astrophysical Journal · 2001 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +14
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469

Centre National de la Recherche Scientifique
Paris, France
26 h-index
89 publications
4.8K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
24 h-index
73 publications
7.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
22 h-index
36 publications
6.2K citations
European Southern Observatory
Garching bei München, Germany
22 h-index
47 publications
4.4K citations
California Institute of Technology
Pasadena, United States
19 h-index
36 publications
3.5K citations

Space Telescope Science Institute
Baltimore, United States
17 h-index
30 publications
2K citations
University of Cambridge
Cambridge, United Kingdom
17 h-index
22 publications
1.4K citations
University of Washington
Seattle, United States
16 h-index
37 publications
3.9K citations
1–8 of 469
ApJ · 142 publications · 16K citations
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62 publications · 3.2K citations
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AJ · 48 publications · 3.2K citations
30
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38 publications · 2.4K citations
28
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PASP · 16 publications · 378 citations
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