X-rag wakes in Abell 160

'Wakes' of X-ray emission have now been detected trailing behind a few (at least seven) elliptical galaxies in clusters. To quantify how widespread th is phenomenon is, and what its nature might be, we have obtained a deep (70 ks) X-ray image of the poor cluster Abell 160 using the ROSAT HRI. Combini ng the X-ray data with optical positions of confirmed cluster members, and applying a statistic designed to search for wake-like excesses, we confirm that this phenomenon is observed in galaxies in this cluster. The probabili ty that the detections arise from chance is less than 3.8 x 10(-3). Further , the wakes are not randomly distributed in direction, but are preferential ly oriented pointing away from the cluster centre. This arrangement can be explained by a simple model in which wakes arise from the stripping of the interstellar media of their host galaxies as a result of ram pressure again st the intracluster medium through which they travel.