Galactic Shear
Galactic Shear is a kinematic phenomenon in galactic dynamics characterized by the differential rotation of adjacent regions of a galaxy, where the relative motion of stars or gas clouds results in a velocity gradient across a given radial distance from the galactic center.
88
Publications
7.5K
Citations
288
Authors
194
Institutions
Publications per year
2017–2026
21
Variants
Galactic Differential Rotation
Parents
88
Christopher M. Hirata, Rachel Mandelbaum, Mustapha Ishak et al. · Monthly Notices of the Royal Astronomical Society · 2007 · 286 citations · Full text
Natural Sciences, Astronomy, Physics +14
Giant Molecular Clouds in M33. II. High‐Resolution Observations
The Astrophysical Journal · 2003 · 212 citations · Full text
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194

Centre National de la Recherche Scientifique
Paris, France
10 h-index
22 publications
2.5K citations
Heidelberg University
Heidelberg, Germany
10 h-index
19 publications
1.7K citations

Australian National University
Canberra, Australia
8 h-index
14 publications
727 citations
University College London
London, United Kingdom
7 h-index
11 publications
1.5K citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
7 h-index
15 publications
1.3K citations
University of Bonn
Bonn, Germany
6 h-index
18 publications
2K citations
University of California, Berkeley
Berkeley, United States
6 h-index
10 publications
1.8K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
6 h-index
15 publications
1K citations
1–8 of 194
29 publications · 3.7K citations
24
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ApJ · 22 publications · 1.4K citations
21
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9 publications · 426 citations
9
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Repository · 4 publications · 481 citations
4
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AJ · 3 publications · 168 citations
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