Abstract

Aims. We measure far-infrared (FIR) emission from tails of stripped dust following the ionised and atomic gas components in galaxies undergoing ram pressure stripping. We study the dust-to-gas relative distribution and mass ratio in the stripped interstellar medium and relate them to those of the intra-cluster medium (ICM), thus linking the cluster-ICM-galaxy evolution at small-scales. The galaxy sample consists of three Scd Virgo galaxies with stellar masses in the range of 10(9)less than or similar to M-*less than or similar to 10(10) M-circle dot and within 1 Mpc from the cluster centre, namely NGC 4330, NGC 4522, and NGC 4654.