Table 3
Parameters of the spectral simulations.
| ID/Parameter | R (× 107 cm) | τ | Lhot (× 1036 erg s-1) | B (× 105 G) | Ld (× 1036 erg s-1) | Tdbb (keV) | Tirr,out (eV) | ||
|
|
|||||||||
| P03 | 1.0 | 2.0 | 25 | 8 | 5.0 | 0.23 | 3.53 | ||
| P18 | 1.5 | 1.7 | 25 | 4 | 2.8 | 0.22 | 2.87 | ||
| IG2 | 3 | 1.5 | 9 | 2 | – | 0.14 | 1.62 | ||
| IG7 | 3 | 1.5 | 11 | 2 | 0.9 | 0.23 | 2.13 | ||
Notes. We adopt MBH = 3M⊙, thus parameters are RS = 8.85 × 105 cm and LEdd = 6 × 1038 erg s-1 (Eddington limit for pure helium). We assumed that Tdbb is equal to the temperature of the injected blackbody photons everywhere except for group IG2 where no seed disk photons were considered. Lhot is the luminosity of the hot flow; it consists of synchrotron, bremsstrahlung, and Comptonized emission.
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