Stellar Radii
Stellar Radii is a metric in astrophysics that quantifies the physical size of stars by measuring the distance from their center to their outermost visible boundary, serving as a fundamental parameter for characterizing stellar structure and evolution.
1.3K
Publications
106.3K
Citations
4.5K
Authors
1K
Institutions
Publications per year
2017–2026
364
Variants
Stellar Radius
Parents
1.3K
Analytic Light Curves for Planetary Transit Searches
Kaisey S. Mandel, Eric Agol · The Astrophysical Journal · 2002 · 2.3K citations · Full text
Natural Sciences, Astronomy, Physics +11
Shrinking Binary and Planetary Orbits by Kozai Cycles with Tidal Friction
The Astrophysical Journal · 2007 · 1.4K citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 1.3K
4.5K
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17
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Center for Astrophysics Harvard & Smithsonian, United States
20 publications · 3.3K citations
17
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1–5 of 4.5K
1K
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
62 h-index
364 publications
48.5K citations
California Institute of Technology
Pasadena, United States
56 h-index
261 publications
31.8K citations

Centre National de la Recherche Scientifique
Paris, France
50 h-index
443 publications
35.1K citations

Ames Research Center
Mountain View, United States
41 h-index
210 publications
55.9K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
37 h-index
95 publications
8.3K citations
University of Arizona
Tucson, United States
36 h-index
111 publications
14K citations
Princeton University
Princeton, United States
36 h-index
90 publications
9.2K citations
University of California, Santa Cruz
Santa Cruz, United States
36 h-index
87 publications
11.5K citations
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ApJ · 399 publications · 39.5K citations
102
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211 publications · 11.9K citations
62
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168 publications · 11.1K citations
57
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AJ · 134 publications · 10K citations
55
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40 publications · 3.5K citations
33
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