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Fig. 5.

image

Spatially resolved map of SFRs in the galaxy HE 1108−2813. On top, we show the bar mask for that galaxy, created from the parameters of the image decomposition and ellipse fitting. The mask is divided into 3 × 9 subcells to analyse how the SFR changes over the bar region. A set of these maps for the complete sample with additional i-band contours can be found in Appendix D.

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