Spectroscopic Variability
Spectroscopic Variability is a systematic change in the spectral characteristics of a star, such as line intensity, shape, or Doppler shift, arising from intrinsic stellar processes or binary orbital motion, as opposed to variations in total electromagnetic flux.
489
Publications
20.4K
Citations
1.9K
Authors
642
Institutions
Publications per year
2017–2026
77
Parents
489
Cygnus X-1—a Spectroscopic Binary with a Heavy Companion ?
B. L. Webster, Paul Murdin · Nature · 1972 · 476 citations
Natural Sciences, Astronomy, Physics +15
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Centre National de la Recherche Scientifique
Paris, France
25 h-index
138 publications
5.5K citations
KU Leuven
Leuven, Belgium
22 h-index
109 publications
4.2K citations
Université Paris Cité
Paris, France
19 h-index
75 publications
3.3K citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
18 h-index
57 publications
2.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
18 h-index
42 publications
2.2K citations

Space Telescope Science Institute
Baltimore, United States
18 h-index
27 publications
1.8K citations
The University of Texas at Austin
Austin, United States
18 h-index
53 publications
2.5K citations

Sorbonne Université
Paris, France
18 h-index
51 publications
2.4K citations
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ApJ · 109 publications · 5.2K citations
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79 publications · 3.2K citations
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85 publications · 3.1K citations
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AJ · 41 publications · 1.7K citations
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16 publications · 563 citations
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