A large H I cloud near the centre of the Virgo cluster

We report the discovery of a large cloud in the central regions of the Virgo cluster. It is kpc in size and contains of . The morphology and kinematics of this cloud strongly suggest that it consists of removed from the galaxy NGC 4388 by ram-pressure stripping. It is more likely the result of an interaction of the ISM of NGC 4388 with the hot halo of the M 86 group and not with the ICM centred on M 87. The large extent of the plume suggests that gas stripped from cluster galaxies can remain neutral for at least 108 yr. Locally, the column density is well above 1020 cm-2, suggesting that the intra-cluster regions known to exist in Virgo may have formed from gas stripped from cluster galaxies. The existence of the plume suggests that stripping of infalling spirals contributes to the enrichment of the ICM. The object in the Virgo cluster recently reported by Minchin et al. (2005, ApJ, 622, L21) may have a similar origin and may therefore not be a “dark galaxy”.