Table 1.
Results.
| Lj (erg s−1) | 1043 | 1044 | 1045 | 1043 | 1044 | 1045 |
|---|---|---|---|---|---|---|
| Γ | 3 | 3 | 3 | 10 | 10 | 10 |
Inverse Compton:  B = 0.1Beq |
||||||
| Lst (erg s−1) | 6.5 × 1039 | 1.7 × 1040 | 1.7 × 1040 | 2.5 × 1039 | 6.9 × 1039 | 1.8 × 1040 |
| Lpop (erg s−1) | 1.1 × 1038 | 6.5 × 1038 | 8.4 × 1038 | 3.7 × 1040 | 4.7 × 1040 | 3.4 × 1040 |
| Ldom (erg s−1) | 1.4 × 1038 | 8.8 × 1037 | 5.5 × 1037 | 3.5 × 1040 | 3.1 × 1040 | 2.5 × 1040 |
| ⟨Mb⟩ (M⊙) | 1.6 × 10−6 | 1.7 × 10−6 | 1.5 × 10−6 | 1.7 × 10−6 | 1.7 × 10−6 | 1.5 × 10−6 |
| ⟨z0⟩ (kpc) | 0.33 | 1.0 | 1.6 | 0.67 | 1.1 | 1.6 |
| PR (yr−1) | 8.3 × 10−3 | 2.6 × 10−2 | 4.0 × 10−2 | 8.6 × 10−3 | 2.7 × 10−2 | 4.0 × 10−2 |
| tobs (yr) | 54 | 170 | 270 | 40 | 33 | 24 |
Synchrotron:  , B = Beq |
||||||
| Lst (erg s−1) | 7.5 × 1041 | 1.9 × 1042 | 1.9 × 1042 | 1.3 × 1041 | 7.4 × 1041 | 2.5 × 1042 |
| Lpop (erg s−1) | 1.4 × 1040 | 4.0 × 1040 | 6.7 × 1040 | 1.1 × 1042 | 2.0 × 1042 | 2.5 × 1042 |
| Lpeak (erg s−1) | 5.8 × 1041 | 5.8 × 1042 | 5.8 × 1043 | 6.3 × 1042 | 6.3 × 1043 | 6.4 × 1044 |
| ⟨Mb⟩ (M⊙) | 1.5 × 10−6 | 1.7 × 10−6 | 1.6 × 10−6 | 1.7 × 10−6 | 1.7 × 10−6 | 1.6 × 10−6 |
| ⟨z0⟩ (kpc) | 0.26 | 0.88 | 1.9 | 0.91 | 1.3 | 1.9 |
| PR (yr−1) | 5.7 × 10−3 | 2.0 × 10−2 | 3.8 × 10−2 | 7.4 × 10−3 | 2.3 × 10−2 | 3.4 × 10−2 |
| tpeak (yr) | 1.3 | 0.14 | 0.014 | 4.8 | 0.48 | 0.046 |
Synchrotron:  , B = Bmin |
||||||
| Bmin (Beq) | 0.02 | 0.01 | 0.01 | 0.04 | 0.03 | 0.02 |
| Lpop (erg s−1) | 2.1 × 1040 | 6.0 × 1040 | 1.4 × 1041 | 1.7 × 1042 | 1.8 × 1042 | 1.4 × 1042 |
| Ldom (erg s−1) | 6.9 × 1040 | 2.1 × 1040 | 4.3 × 1040 | 1.8 × 1042 | 1.1 × 1042 | 1.9 × 1042 |
| tobs (yr) | 13 | 45 | 32 | 38 | 65 | 10 |
Notes. Results for the emission of the whole population of red giants interacting with the jet in steady state (Lst) and through injecting bubbles at penetration (Lpop), respectively; Ldom is the luminosity of the typical bubble event that dominates the aforementioned emission, and below it the characteristics of this event are given. For six different jet configurations, we list all results in three cases: inverse Compton emission of electrons with energy 
for B = 0.1Beq, and synchrotron emission at 100 MeV for Beq and Bmin. The non-listed characteristics of the dominant event in the case of synchrotron emission with Bmin are the same as those of the emission with Beq, for each jet configuration. All the luminosities and energies scale with η/0.1 ≤ 10. The luminosities and times are as seen by the observer.
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