Distribution of star formation in galactic bars as seen with Hα and stacked GALEX UV imaging
            
    Context. Stellar bars are known to gradually funnel gas to the central parts of disk galaxies. It remains a matter of debate why the distribution of ionized gas along bars and in the circumnuclear regions varies among galaxies. Aims: Our goal is to investigate the spatial distribution of star formation (SF) within bars of nearby low-inclination
            Díaz-García, S. et al.
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                        2020