Table 2.
Properties of 3C 59.
| Source properties | Ref. | |
|---|---|---|
| (1) | MBH = 108.9 M⊙ | Wu & Liu (2004) |
| (2) | Lbol = 3.45 × 1045 erg s−1 | Section 4.1 |
| (3) | LEdd = 1.02 × 1047 erg s−1 | Section 4.1 |
| (4) | λEdd = 0.03 | Section 4.1 |
| (5) | Lion = 1.79 × 1045 erg s−1 | Section 4.1 |
| (6) | Ṁacc = 0.62 M⊙ yr−1 | Section 4.1 |
| (7) | 0.009 pc ≲ RBLR ≲ 0.03 pc | Section 4.3 |
| (8) | 0.7 pc ≲ Rtorus ≲ 22 pc | Section 4.3 |
| (9) | RNLR ≲ 9 kpc | Section 4.3 |
| WAH properties | Ref. | |
| (10) | 25 pc ≲ r ≲ 188 pc | Section 4.3 |
| (11) | Ṗabs = 1.28 × 1035 erg m−1 | Section 4.6 |
| (12) | Ṗscatt = 2.73 × 1034 erg m−1 | Section 4.6 |
| (13) | Ṁout = 0.47 M⊙ yr−1 | Section 4.6 |
| (14) | ĖK = 4.11 × 1040 erg s−1 | Section 4.6 |
| WAL properties | Ref. | |
| (15) | 135 pc ≲ r ≲ 4 kpc | Section 4.3 |
| (16) | Ṗabs = 4.43 × 1035 erg m−1 | Section 4.6 |
| (17) | Ṗscatt = 1.22 × 1034 erg m−1 | Section 4.6 |
| (18) | Ṁout = 3.15 M⊙ yr−1 | Section 4.6 |
| (19) | ĖK = 5.20 × 1040 erg s−1 | Section 4.6 |
Notes. (1): Black hole mass; (2): Bolometric luminosity; (3): Eddington luminosity; (4): Eddington ratio; (5): 1−1000 Ryd ionizing luminosity; (6): Mass accretion rate; (7): Distance of BLR to BH; (8): Distance of dust torus to BH; (9): Distance of NLR to BH; (10) and (15): Distance of warm absorbers to BH; (11) and (16): Momentum of radiation being absorbed by warm absorbers; (12) and (17): Momentum of radiation being scattered by warm absorbers; (13) and (18): Mass outflow rate of warm absorbers; (14) and (19): Kinetic energy of warm absorbers.
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