Rotating Variable Stars
Rotating Variable Stars is a class of variable stars whose observed brightness variations are primarily caused by the rotational modulation of surface features such as starspots, ellipsoidal deformations, or brightness inhomogeneities, distinguishing them from pulsating or eclipsing variable stars.
75
Publications
5K
Citations
284
Authors
132
Institutions
Publications per year
2017–2026
8
Variants
Rotational Variables
Parents
75
Bill Paxton, R. Smolec, Josiah Schwab et al. · The Astrophysical Journal Supplement Series · 2019 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
Some remarks on the variable stars in globular clusters
P.T. Oosterhoff · Observatory · 1939 · 179 citations
Natural Sciences, Astronomy, Physics +14
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2 publications · 92 citations
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2
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132
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
9 publications
255 citations

University of Warsaw
Warsaw, Poland
5 h-index
20 publications
410 citations
University of Liège
Liège, Belgium
4 h-index
13 publications
350 citations
California Institute of Technology
Pasadena, United States
3 h-index
5 publications
190 citations
KU Leuven
Leuven, Belgium
3 h-index
3 publications
248 citations
South African Radio Astronomy Observatory
Cape Town, South Africa
3 h-index
4 publications
199 citations

University of Wrocław
Wroclaw, Poland
3 h-index
6 publications
148 citations
American Institute of Aeronautics and Astronautics
Reston, United States
2 h-index
2 publications
38 citations
1–8 of 132
ApJ · 22 publications · 1K citations
17
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10 publications · 363 citations
10
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AJ · 11 publications · 502 citations
10
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CoAst · 6 publications · 167 citations
6
h-index
5 publications · 230 citations
5
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1–5