Open Access

Table 1.

Parameters that were varied in a set of seven simulations to showcase diverse jet environment conditions.

Simulation Jet radius Jet velocity Jet B-field Jet flow along Domain (kpc) Grid Remarks
label (rj in pc) (Γ) (σ) environment’s [x], [y], [z]
Major axis [ − 12,  12] 576 low B-field
lowB_maj5 200 3 0.01 (Θ = 5°) [ − 16,  16] 768 cases ↓
[ − 12,  12] 576

intermediate variation in flow
lowB_intm40 200 3 0.01 axis as above as above axis
(Θ = 40°)

variation in flow
lowB_min85 200 3 0.01 minor axis as above as above axis
(Θ = 85°)

[ − 6,  6] 556 variation in rj, vj,
lowB_varRV_min85 108 5 0.01 minor axis [ − 16,  16] 1482 but raising same jet
(Θ = 85°) [ − 6,  6] 556 power as others

highB_maj5 200 3 0.1 major axis same as same as High B-field
(Θ = 5°) top row top row cases ↓

intermediate
highB_intm40 200 3 0.1 axis same as same as variation in flow
(Θ = 40°) top row top row axis

highB_min85 200 3 0.1 minor axis same as same as variation in flow
(Θ = 85°) top row top row axis

Notes. The first column lists the simulation labels, identifying the unique attributes of each case. Columns 2–4 detail the jet injection radius, velocity, and magnetic field strength, respectively. These parameters were carefully selected to maintain a constant jet power across all cases, which allows investigation into whether intrinsic parameters, rather than jet power, drive radio galaxy evolution. Column 5 describes the jet’s propagation relative to the axis of the ambient medium. Columns 6 and 7 specify the computational domain and grid distribution, ensuring that five grid cells are allocated per jet injection radius. Finally, remarks for each case are included in the last column for clarity. The jet–to–ambient density contrast is fixed at 10−6 in all of these cases.

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