HI deficiency (top row) and H₂ deficiency (bottom row) plotted against local densities for Virgo filament galaxies (center), AMIGA isolated galaxies (left), and Virgo cluster galaxies (right). Triangles show the binned median values, while their error bars correspond to the rms dispersion around the median; equally, equally spaced bins, in log scale, with at least five points each have been considered. Sources are color coded according to their morphological de Vaucouleurs classification.