We report the discovery of bent double jets in the elliptical galaxy NGC 1272 , a member of the Perseus cluster .
The jets have a radius of curvature of \sim 2 kpc , much smaller than the galaxy half-light radius of \sim 11 kpc .
This bending is likely a result of ram pressure , and indicates that the intracluster gas enters deep within the galaxy and that the interstellar medium of NGC 1272 has been significantly removed .
X-ray observations of the surrounding intracluster medium allow us to constrain the pressure within the jet .
We find that the standard assumptions of equipartition often used in interpreting other jets underestimate the pressure in the jets by a factor \sim 30 .