Rotational Broadening
Rotational Broadening is a spectroscopic phenomenon in stellar astronomy whereby the spectral lines of a rotating star are widened due to the Doppler shifts arising from the differential line-of-sight velocities across the star’s rotating surface.
276
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14.1K
Citations
906
Authors
376
Institutions
Publications per year
2017–2026
46
Parents
276
Fundamental photon noise limit to radial velocity measurements
F. Bouchy, F. Pepe, D. Queloz · Astronomy and Astrophysics · 2001 · 428 citations
Natural Sciences, Astronomy, Physics +17
Measurement of Spin‐Orbit Alignment in an Extrasolar Planetary System
Joshua N. Winn, R. W. Noyes, Matthew J. Holman et al. · The Astrophysical Journal · 2005 · 349 citations · Full text
Natural Sciences, Astronomy, Physics +13
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376
Instituto de Astrofísica de Canarias
Tenerife, Spain
20 h-index
49 publications
2.3K citations

Centre National de la Recherche Scientifique
Paris, France
20 h-index
69 publications
5.9K citations

University of Warwick
Coventry, United Kingdom
17 h-index
31 publications
1.2K citations
Osservatorio Astrofisico di Catania
Catania, Italy
17 h-index
91 publications
3K citations
Osservatorio Astronomico di Palermo
Palermo, Italy
16 h-index
91 publications
2.9K citations
Osservatorio Astronomico di Padova
Padua, Italy
16 h-index
134 publications
4.3K citations
Telescopio Nazionale Galileo
Garafía, Spain
16 h-index
140 publications
5K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
16 h-index
26 publications
1.5K citations
1–8 of 376
ApJ · 75 publications · 4K citations
37
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52 publications · 2.5K citations
26
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27 publications · 1.7K citations
22
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15 publications · 969 citations
14
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AJ · 15 publications · 1.3K citations
14
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