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Home All issues Volume 661 (May 2022) A&A, 661 (2022) A98 Full HTML
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Fig. 2.

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Dependence of central sSFR (sSFRfiber) on strength of spiral arms (2 + log sarm). Panel a: the scatter plot of the two parameters. Panel b: shows the number distribution of sSFRfiber. The solid horizon line (logsSFRfiber = −11.3) marks the valley of the number distribution, separating the sample into centrally star-forming and centrally quenched SFMS galaxies. The Pearson correlation coefficient between sSFRfiber and 2 + log sarm is denoted at the top.

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