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Fig. 4

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The dust-to-stellar mass ratio as function of stellar mass (top row), NUV − r colour (middle row), and stellar mass surface density (bottom row) for HI-normal (first column), HI-deficient (second column) galaxies, systems outside (third column) and inside (fourth column) the Virgo cluster. Circles and black triangles indicate detections and non-detections respectively. The average relations for HI-normal (solid), HI-deficient (long-dashed) galaxies, systems outside (dotted) and inside (short dashed) the Virgo cluster are presented in the fifth column. In the third and fourth column Hi-deficient galaxies outside the Virgo cluster and Hi-normal Virgo galaxies are highlighted in red and blue, respectively.

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