Fig. 4.

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Distribution of SFRD in the identified regions of the inner ring of the galaxy (region shown in the inset of Fig. 1) based on their angles relative to north in a boxplot. The box represents the interquartile range of the observed SFRD, the orange stars indicate the median of the SFRD, and the whiskers depict data points within the range of 1.5 times the interquartile range. Outliers, depicted as green diamonds beyond the whisker limits, are values that fall outside this range. Individual hyphen markers in some places indicate that only a single star-forming region subtends the corresponding angle. We observe a peak in the SFRD at the area of the inner ring in conjunction with the ends of the bar.
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