Bar-driven Spiral Structure
Bar-Driven Spiral Structure is a theoretical astrophysical model within galactic dynamics that specifies spiral arm formation in disk galaxies as primarily induced and sustained by non-axisymmetric gravitational perturbations originating from a central stellar bar.
57
Publications
3.8K
Citations
160
Authors
131
Institutions
Publications per year
2017–2026
7
Parents
57
The response of gas in a galactic disk to bar forcing
M. P. Schwarz · The Astrophysical Journal · 1981 · 322 citations
Natural Sciences, Astronomy, Physics +17
On a mechanism that structures galaxies
D. Lynden–Bell · Monthly Notices of the Royal Astronomical Society · 1979 · 195 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 57
160
4
h-index
3
h-index
Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France
3 publications · 191 citations
3
h-index
3
h-index
2
h-index
1–5 of 160
131

Centre National de la Recherche Scientifique
Paris, France
8 h-index
25 publications
2.4K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
5 h-index
6 publications
570 citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
4 h-index
11 publications
232 citations
Heidelberg University
Heidelberg, Germany
4 h-index
8 publications
724 citations
The University of Tokyo
Tokyo, Japan
3 h-index
5 publications
655 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
3 h-index
7 publications
1.1K citations
Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères
Paris, France
3 h-index
3 publications
285 citations
Galaxies, Etoiles, Physique et Instrumentation
Meudon, France
3 h-index
9 publications
701 citations
1–8 of 131
19 publications · 1.4K citations
18
h-index
ApJ · 16 publications · 1.1K citations
14
h-index
5 publications · 369 citations
5
h-index
AJ · 4 publications · 208 citations
4
h-index
2 publications · 107 citations
2
h-index
1–5