Radial Velocity Variability
Radial Velocity Variability is the systematic variation in the line-of-sight component of a star's motion relative to an observer, as measured through Doppler shifts in spectral lines, that arises from intrinsic astrophysical processes such as rotational modulation, pulsations, accretion dynamics, or the presence of unseen companions during the pre-main sequence evolutionary phase.
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Astronomy and Astrophysics · 2001 · 745 citations · Full text
Natural Sciences, Astronomy, Physics +16
Activity‐Related Radial Velocity Variation in Cool Stars
Steven H. Saar, R. A. Donahue · The Astrophysical Journal · 1997 · 537 citations · Full text
Natural Sciences, Astronomy, Physics +16
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
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161 publications
14.5K citations

Centre National de la Recherche Scientifique
Paris, France
36 h-index
285 publications
23.9K citations
University of Geneva
Geneva, Switzerland
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252 publications
24.6K citations
The University of Texas at Austin
Austin, United States
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112 publications
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European Southern Observatory
Santiago, Chile
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University of California, Berkeley
Berkeley, United States
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Instituto de Astrofísica de Canarias
Tenerife, Spain
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6.5K citations
Thüringer Landessternwarte Tautenburg
Tautenburg, Germany
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ApJ · 201 publications · 13.4K citations
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AJ · 72 publications · 3.2K citations
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Repository · 22 publications · 757 citations
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