Fig. 5.
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B. Continued. Intensity maps (log Iν) at 1 GHz radio frequency depicting the X-shaped radio galaxy in their giant stages, resulting from jet propagation along the direction of highest jet frustration (i.e., along the major axis direction). The low jet power case (“GRG_lp_maj”; top) and the high jet power case (“GRG_hp_maj”; bottom) exhibit distinct decollimation patterns, with both cases generating internal regions of emission valleys and enhanced emission ridges. The wings are luminous, indicating their active evolutionary stages (∼196 Myr: top; ∼137 Myr: bottom).
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