Rotation-age Relations
Rotation-Age Relations is a theoretical framework in astrophysics that establishes a predictive correlation between the rotational periods of stars and their ages, enabling stellar age estimation through observed rotational properties.
203
Publications
16.2K
Citations
711
Authors
341
Institutions
Publications per year
2017–2026
52
Variants
Gyrochronology
Parents
203
1–5 of 203
711
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341
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
17 h-index
46 publications
5.2K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
55 publications
6.9K citations
California Institute of Technology
Pasadena, United States
12 h-index
20 publications
1.5K citations
Space Science Institute
Boulder, United States
11 h-index
12 publications
687 citations
Columbia University
New York, United States
10 h-index
23 publications
1.6K citations
Université Paris Cité
Paris, France
9 h-index
24 publications
1.6K citations
The Ohio State University
Columbus, United States
9 h-index
18 publications
1.9K citations
Princeton University
Princeton, United States
9 h-index
13 publications
990 citations
1–8 of 341
ApJ · 54 publications · 5.8K citations
39
h-index
27 publications · 1.8K citations
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19 publications · 1.8K citations
18
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AJ · 16 publications · 920 citations
15
h-index
8 publications · 807 citations
8
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1–5