Table 2
Adopted parameters for the hot spot and lobe models shown in Figs. 6 and A.3.
| Model [1] | Comp. [2] | R [3] | θV [4] | β [5] | Pe,45 [6] | B [7] | γb [8] | γmax [9] | log Ee [10] | log EB [11] | Ee/Eb [12] |
|---|---|---|---|---|---|---|---|---|---|---|---|
| A | HS | 1 | 3°, −177° | 0.06 | 2.3 | 180 | 600 | 1e6 | 56.2 | 56.2 | 0.9 |
| A | lobe | 20 | – | 0 | 50 | 7 | 300 | 1e5 | 59.2 | 57.3 | 89 |
| B | HS | 2 | 3°, −177° | 0.06 | 5.4 | 140 | 600 | 1e6 | 56.9 | 56.9 | 1 |
| B | lobe | 20 | – | 0 | 50 | 2.4 | 300 | 1.e5 | 59.2 | 56.4 | 630 |
| C | HS | 2.9 | 3°, −177° | 0.06 | 600 | 7 | 400 | 1.e4 | 59.4 | 54.8 | 4e4 |
| D | HS | 2.9 | 3°, −177° | 0.06 | 600 | 7 | 400 | 1.e4 | 59.4 | 54.8 | 4e4 |
| D | lobe | 20 | – | 0 | 1 | 12 | 400 | 1e4 | 57.8 | 57.7 | 1.2 |
Notes. Column [1]: Type of model; Col. [2]: component (HS = hot spot); Col. [3]: size in kpc; Col. [4]: viewing angle; Col. [5]: bulk velocity; Col. [6]: Power injected in relativistic electrons in units of 1045 erg s−1; Col. [7]: magnetic field in μG; Cols. [8] and [9]: break and maximum Lorenz factor of the injected electron distribution; Col. [10]: logarithm of the total energy in relativistic electrons, in erg; Col. [11]: logarithm of the total energy in magnetic field, in erg; Col. [12]: total energy in relativistic electrons over total energy in magnetic field. The values of the powers and the energetics refer to each hot spot and lobe. The lobe flux shown in the figures corresponds to two lobes. We assume to inject throughout the source Q(γ) relativistic electrons with a broken power law distribution, i.e. Q(γ) ∝ γ below γ = γb and Q(γ) ∝ γ−27 between γb and γmax.
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