Table 4.
Inferred wind parameters in our sample (plus the published results).
| Names | log Rw | log nH | log Ṁout | log Lkin | [CV] (a) | Lkin/LEdd(b) |
|---|---|---|---|---|---|---|
| (cm) | (cm−3) | (g s−1) | (erg s−1) | (10−3) | % | |
| This work | ||||||
| 1H 1934-063 | 13.8 − 18.8(17.1) | 2.6(6⋆)−12.6 | 21.6(23.3)−26.6 | 40.4(42.1)−45.4 | 9.0 ± 2.4 | 6.8 × 10−3(0.4)−7.6 × 102 [3.5 ± 2.0] |
| RE J1034+396 | 13.3 − 19.9(17.6) | 1.6(6⋆)−14.7 | 21.4(23.6)−27.9 | 40.6(42.8)−47.2 | 7.1 ± 2.6 | 1.2 × 10−2(2.1)−4.7 × 104 [26.0 ± 18.6] |
| PG 1244+026 | 15.3 − 22.8(18.5) | −2.6(6⋆)−12.4 | 21.5(25.8)−29.0 | 39.4(43.7)−47.0 | 0.7 ± 0.2 | 1.6 × 10−4(3.4)−5.6 × 103 [1.0 ± 0.5] |
| PG 1211+143 | 16.1 − 22.2(18.4) | −1.6(6⋆)−10.6 | 22.9(26.7)−29.0 | 41.0(44.8)−47.1 | 1.2 ± 0.4 | 5.8 × 10−4(3.6)−7.3 × 102 [0.4 ± 0.2] |
| PG 1211+143-2 | 16.5 − 22.2(18.2) | −2.1(6⋆)−9.3 | 22.6(26.6)−28.3 | 40.4(44.4)−46.1 | 5.6 ± 2.1 | 1.3 × 10−4(1.3)−6.2 × 101 [0.15 ± 0.09] |
| I ZW 1 | 14.3 − 16.2(17.2) | 7.9(6⋆)−11.8 | 25.2(24.2)−27.1 | 44.4(43.4)−46.3 | 71.2 − 26.6 | 7.0 × 100(0.8)−5.7 × 102 [17.8 ± 9.0] |
| I ZW 1-2 | 15.1 − 22.8(18.5) | −2.7(6⋆)−12.8 | 21.5(25.8)−29.2 | 40.0(44.3)−47.7 | 0.5 ± 0.2 | 2.8 × 10−4(6.0)−1.5 × 104 [3.2 ± 2.0] |
| IRAS 17020+4544 | 14.4 − 22.8(18.6) | −2.4(6⋆)−14.4 | 21.1(25.3)−29.5 | 39.6(43.7)−47.9 | 0.2 ± 0.1 | 5.4 × 10−4(8.2)−1.3 × 105 [3.6 ± 1.7] |
| Published work | ||||||
| Mrk 1044 (c) | 13.6 − 15.4 | 9.0 − 12.6 | 24.2 | 43.2 | 7.0 | 4.4 |
| 1H 0707-495 (d) | 13.4 − 14.8 | 10.7 − 13.0 | 24.5 | 43.4 | 8.0 | 13.7 |
| IRAS 13224−3809 (e)(f) | 13.6 − 14.2 | 10 − 12 | 24.4 | 43.4 | 3.8 | |
| PDS 456 (g) | 16.2 − 16.8 | 6.5 − 8.9 | 27.1 | 46.3 | 15.0 | |
Notes. The inferred parameters are calculated by assuming a solid angle of Ω/4π = 0.3 (Tombesi et al. 2010; Takeuchi et al. 2013). ⋆The lower limit on the density is assumed above the typical density of narrow line region (NLR, > 106 cm−3). The corresponding results are shown in parentheses.
The filling factor is calculated by assuming that the outflow rate is comparable to the accretion rate Ṁout ∼ Ṁacc (Kobayashi et al. 2018).
The value in the bracket is estimated by inputting CV into Eq. (4) based on assumption of Ṁout ∼ Ṁacc.
References.
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