Table 1.
Characteristic parameters of our simulation runs.
| ID | Simulation inputs | ṁ from SED fits | Comments | |||||
|---|---|---|---|---|---|---|---|---|
| β0 | ρflr | uflr | a | Risco | ṁHIGH−mass | ṁLOW−mass | ||
| SIM20 | 10 | 10−5 | 10−8 | 0.9375 | 2 Rg | 2.0×10−5 | 5.6×10−7 | reference run, similar to Vourellis et al. (2019) |
| SIM21 | 10 | 10−4 | 10−6 | 0.9375 | 2 Rg | 1.0×10−5 | 5.0×10−7 | as SIM20, floor density higher |
| SIM22 | 10 | 10−4 | 10−6 | 0.0 | 6 Rg | 7.0×10−5 | 5.0×10−6 | as SIM20, a = 0, infall to BH, disk wind |
| SIM23 | 10 | 10−3 | 10−5 | 0.9375 | 2 Rg | 3.0×10−6 | 1.5×10−7 | as SIM21, floor even higher, no BZ |
| SIM24 | 1 | 10−3 | 10−5 | 0.9375 | 2 Rg | 4.0×10−7 | 2.0×10−8 | as SIM21, β0 lower, stronger magn. field |
| SIM26 | 0.1 | 10−3 | 10−5 | 0.9375 | 2 Rg | 2.0×10−7 | 1.0×10−8 | as SIM24, β0 even lower, even stronger magn. field |
Notes. Shown here: the simulation ID, the initial disk plasma beta, β0 (at the inner disk radius), the maximum floor density, ρflr, and internal energy, uflr, the Kerr parameter of the BH, a, the radius of the ISCO, Risco, and specific comments on the simulation runs, respectively. The Eddington ratios of these simulations for the defined HIGH-mass and LOW-mass system are obtained from the SED fits to the data for M87 as tabulated in Prieto et al. (2016) and for SgrA* in Narayan et al. (1998). The fits are obtained by fixing the values of Rlow = 1, Rhigh = 80 and an inclination angle of i = 17° when postprocessing the simulated data for each of the models.
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