  We have investigated how varying several parameters affects the results of a
collision between an extragalactic jet and a dense, intergalactic cloud,
through a series of hydrodynamic simulations. We have produced synthetic radio
images for comparison with observations. These show that a variety of
structures may be produced from simple jet-cloud collisions. Moderate Mach
numbers and density contrasts are needed to produce observable bends. We
investigate the effect of viewing from various angles on the appearance of such
sources.
