Multi-arm Spiral Patterns
Multi-Arm Spiral Patterns is a theoretical construct in galactic astronomy that describes the coherent, large-scale organization of spiral density waves in disk galaxies characterized by the presence of two or more dominant spiral arms originating from the galactic center, distinguishing it from single-arm or flocculent spiral configurations by its higher symmetry and arm multiplicity.
39
Publications
1.9K
Citations
96
Authors
58
Institutions
Publications per year
2017–2026
4
Parents
39
SELF-PERPETUATING SPIRAL ARMS IN DISK GALAXIES
The Astrophysical Journal · 2013 · 224 citations · Full text
Natural Sciences, Astronomy, Physics +16
THE EFFECT OF RADIAL MIGRATION ON GALACTIC DISKS
The Astrophysical Journal · 2014 · 121 citations · Full text
Natural Sciences, Astronomy, Physics +16
The effect of radial migration on galactic disks
Carlos Vera-Ciro, Elena D’Onghia, Julio F. Navarro et al. · CONICET Digital (CONICET) · 2014 · 110 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 39
96
2
h-index
2
h-index
2
h-index
1
h-index
1
h-index
1–5 of 96
58

University of Victoria
Victoria, Canada
2 h-index
2 publications
231 citations

Chinese Academy of Sciences
Beijing, China
2 h-index
3 publications
81 citations
Miller College
Battle Creek, United States
2 h-index
2 publications
36 citations

Universidad Nacional de Córdoba
Córdoba, Argentina
2 h-index
2 publications
231 citations
Argentine National Observatory
Córdoba, Argentina
2 h-index
2 publications
231 citations
National Research Council Canada
Ottawa, Canada
2 h-index
2 publications
140 citations

Cornell University
Ithaca, United States
2 h-index
3 publications
218 citations
University of California, Berkeley
Berkeley, United States
2 h-index
2 publications
36 citations
1–8 of 58
ApJ · 11 publications · 710 citations
11
h-index
7 publications · 297 citations
7
h-index
AJ · 5 publications · 321 citations
5
h-index
Repository · 1 publications · 18 citations
1
h-index
CTP · 1 publications · 10 citations
1
h-index
1–5