Arm Interarm Contrast
Arm Interarm Contrast is a quantitative metric in galactic astronomy that measures the relative density or brightness difference between the spiral arms and the interarm regions of a galaxy, thereby characterizing the prominence of spiral structure in the context of Milky Way Structure.
35
Publications
2.5K
Citations
130
Authors
84
Institutions
Publications per year
2017–2026
3
Parents
35
Nonaxisymmetric Structures in the Stellar Disks of Galaxies
The Astrophysical Journal · 1995 · 297 citations · Full text
Natural Sciences, Astronomy, Physics +14
Jane Huang, Sean M. Andrews, Laura M. Pérez et al. · The Astrophysical Journal Letters · 2018 · 173 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 35
130
4
h-index
3
h-index
2
h-index
2
h-index
2
h-index
1–5 of 130
84
Max Planck Institute for Astronomy
Heidelberg, Germany
3 h-index
5 publications
253 citations

Kitt Peak National Observatory
Tucson, United States
3 h-index
4 publications
204 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
3 h-index
6 publications
787 citations
Association of Universities for Research in Astronomy
Washington, United States
3 h-index
4 publications
204 citations

U.S. National Science Foundation
Alexandria, United States
3 h-index
4 publications
204 citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
3 h-index
6 publications
320 citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
3 h-index
15 publications
1.2K citations
Max Planck Institute for Astrophysics
Garching, Germany
2 h-index
2 publications
203 citations
1–8 of 84
ApJ · 10 publications · 580 citations
11
h-index
AJ · 5 publications · 231 citations
5
h-index
4 publications · 283 citations
4
h-index
3 publications · 289 citations
3
h-index
3 publications · 186 citations
3
h-index
1–5