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Figure 11
.
First row are the 4 original images of galaxies with single spiral-ring patterns: a: unknown-name ring 1 from reference [24], b: unknown-name ring 2 from reference [24], c: ESO 325-28; d: NGC 2273. Second row are the images with simulations by the ROTASE model for each related original galaxies in the first row, e: ρ = 0.5, Euler(6,0,0); f: ρ = 0.5, Euler(-25,40, 55); g: ESO 325-28, ρ = 0.65; h: NGC 2273, ρ = 0.6, Euler (-43, 57, 80)
From
Spirals and Rings in Barred Galaxies by the ROTASE Model
Hongjun Pan
International Journal of Physics
.
2021
, 9(6), 286-307 doi:10.12691/ijp-9-6-5
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