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This article has an erratum: [https://doi.org/10.1051/0004-6361/201219200e]


Fig. 13

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The distribution of the Balmer decrement C(Hβ) or A(Hα) for the whole the HRS sample (above) and excluding AGNs (below). The black line indicates the whole sample of late-type galaxies, the blue line that of galaxies with a normal HI gas content (HI − def ≤ 0.4) and the red one that of HI-deficient Virgo cluster objects (HI − def > 0.4).

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