Oort Constants
Oort Constants is a pair of derived parameters in galactic kinematics that quantify the local rotational properties of the Milky Way, specifically characterizing the shear and vorticity of the galactic rotation field in the solar neighborhood.
43
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3.2K
Citations
84
Authors
58
Institutions
Publications per year
2017–2026
4
Parents
43
Refining the Oort and Galactic constants
Monthly Notices of the Royal Astronomical Society · 1998 · 128 citations · Full text
Natural Sciences, Astronomy, Physics +14
Galactic rotation in <i>Gaia</i> DR1
Jo Bovy · Monthly Notices of the Royal Astronomical Society Letters · 2017 · 125 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 43
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Instituto de Química del Noroeste Argentino, Argentina
3 publications · 38 citations
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2
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2
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2
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1–5 of 84
58
Institute of Astronomy
Moscow, Russia
3 h-index
3 publications
208 citations
Instituto de Química del Noroeste Argentino
San Miguel de Tucumán, Argentina
3 h-index
3 publications
38 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
3 publications
272 citations

University of Toronto
Toronto, Canada
3 h-index
3 publications
244 citations

Australian National University
Canberra, Australia
2 h-index
2 publications
183 citations
United States Naval Observatory
Flagstaff, United States
2 h-index
2 publications
113 citations
National Astronomical Observatories
Beijing, China
2 h-index
4 publications
115 citations

University of Ljubljana
Ljubljana, Slovenia
2 h-index
2 publications
183 citations
1–8 of 58
16 publications · 919 citations
14
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ApJ · 10 publications · 1.5K citations
10
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AJ · 5 publications · 262 citations
5
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Repository · 2 publications · 31 citations
2
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1 publications · 25 citations
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1–5