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The effects of bar–spiral coupling on stellar kinematics in the Galaxy

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Academic year: 2021

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Figure

Table 1. Amplitudes of the perturbation potentials presented in this work.
Figure 2. Profiles for the disc test particles density at t = 0 (blue dots), and the volume density ρ thin of the thin disc (red line) of Model I by Binney
Figure 3. Top: power spectrum √
Figure 4. Average velocities at t = t e for the simulation B on x versus y plane. Left-hand panel: v R
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