Fig. A.1.
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Temporal evolution of C2, z, b/p strength computed from the Fourier decomposition using Eq. A.1, plotted against the b/p strength calculated using Eq. 1 for the model rthickE0.5. All the stellar particles (thin+thick) within the b/p extent (Rb/p) are used in both cases. The colour bar denotes the time of the simulation. Both the measures of b/p strength correlate fairly well.
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