Fig. 11.
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ΣSFR in the nuclear disc with respect to bar ageing. We present the measured median ΣSFR in the nuclear disc region (as defined in this work; see Table 3) for different bar ages, finding a strong anti-correlation (r=−0.791±0.003 and p-value = 0.0011±0.0003). This demonstrates that, as the bar ages, the nuclear discs tend to form fewer stars.
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