Table 2.
Parameters of the different scenarios calculated for the model.
| Scenario |
|||||
|---|---|---|---|---|---|
| Parameter | Symbol [units] | S1 | S2 | S3 | S4 |
| Black hole mass (1) | MBH [M⊙] | 5 | 5 | 20 | 20 |
| Mass accretion rate (1) | Ṁinput [M⊙ yr−1] | 1.1 × 10−5 | 1.1 × 10−4 | 4.4 × 10−5 | 4.4 × 10−4 |
| Orbital semi-axis (1) | a [R⊙] | 15 | 15 | 22 | 22 |
| Gravitational radius (2) | rg [cm] | 7.4 × 105 | 7.4 × 105 | 2.9 × 106 | 2.9 × 106 |
| Critical radius (2) | rcrit [rg] | 4000 | 40 000 | 4000 | 40 000 |
| Mass loss in disk winds (1) | Ṁdw [M⊙ yr−1] | 10−5 | 10−4 | 4.3 × 10−5 | 4.3 × 10−4 |
| Kinetic power of the disk-driven wind (2) |
 [erg s−1] |
7.8 × 1039 | 7.8 × 1040 | 3.4 × 1040 | 3.4 × 1041 |
| Cold matter density at SP (2) | ndw [cm−3] | 5.1 × 1012 | 5.1 × 1013 | 2.9 × 1012 | 2.9 × 1013 |
| Distance to SP from BH (2) | rBH [cm] | 2.7 × 1011 | 2.7 × 1011 | 7.6 × 1011 | 7.6 × 1011 |
| Size of acceleration region (1) | Δxac [cm] | 2.7 × 1010 | 2.7 × 1010 | 7.6 × 1010 | 7.6 × 1010 |
| Shock cold matter density (2) | nRS [cm−3] | 2 × 1013 | 2 × 1014 | 1.2 × 1013 | 1.2 × 1014 |
| Shock cooling length (2) | RΛ [cm] | 7.6 × 1011 | 7.6 × 1010 | 1.3 × 1012 | 1.3 × 1011 |
| Maximum energy of electrons (2) |
 [eV] |
1011 | 1.6 × 1011 | 1011 | 1011 |
| Maximum energy of protons (2) |
 [eV] |
1015 | 1015 | 3 × 1015 | 3.1 × 1015 |
| Emission peak (low energy) (2) | L0.01 mm [erg s−1] | 3.2 × 1033 | 3.2 × 1033 | 8 × 1034 | 8 × 1034 |
| Emission peak (high energy) (2) | L10 MeV [erg s−1] | 4 × 1032 | 4 × 1032 | 1034 | 1034 |
Notes. We indicate with superscript (1) those parameters that are assumed and with (2) those that are derived. In all models, the system is supposed to be oriented face-on to the observer, that is, the inclination of the normal to the orbital plane i with respect to the line of the sight is ∼0°.
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