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We examine two members of the NGC 4065 group of galaxies: a bent‐double (aka wide angle tail) radio source and an H  i ‐deficient spiral galaxy. Models of the X‐ray‐emitting intragroup gas and the bent‐double radio source, NGC 4061, are used to probe the density of intergalactic gas in this group. H  i  observations reveal an asymmetric, truncated distribution of H  i  in spiral galaxy, UGC 07049, and the accompanying radio continuum emission reveals strong star formation. We examine the effectiveness of ram‐pressure stripping as a gas‐removal mechanism and find that it alone cannot account for the H  i  deficiency that is observed in UGC 07049 unless this galaxy has passed through the core of the group with a velocity of . A combination of tidal and ram‐pressure stripping are necessary to produce the H  i  deficiency and asymmetry in this galaxy.

Quantifying the importance of ram‐pressure stripping in a galaxy group at 100 Mpc