Traces of the evolution of cosmic void galaxies: An integral field spectroscopy-based analysis

Open Access

Fig. 7.

Profiles of the mean stellar metallicity (top panels) and stellar age (bottom panels). The left-hand panels correspond to ETGs, and the right-hand panels to LTGs. Void galaxies are shown with dashed red lines, while non-void galaxies are shown with solid gray line. Error bars indicate the uncertainty in the mean, calculated as $σ / \sqrt{n}$ $\sigma/\sqrt{n}$ . (a) ETGs. (b) LTGs.

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