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Home All issues Volume 665 (September 2022) A&A, 665 (2022) A93 Full HTML
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Table 2.

Photoionized models of the absorption and emission components.

C99 X01 C02 C05 C07 C13 X13s X13w X14 X16 X21
Obscuration component 1
NH (1025 m−2) − − − − − 11.7 ± 0.2 12.4 ± 0.1 10.7 ± 0.3 11.4 ± 0.3 15.4 ± 0.5 11.3 ± 0.4
log(ξ) (10−9 W m) − − − − − 0.71 ± 0.05 −0.08 ± 0.04 −4.0(f) −1.97 ± 0.32 −1.57 ± 0.62 0.97 ± 0.04
Cabs − − − − − 0.95 ± 0.05 0.94 ± 0.02 0.84 ± 0.03 0.96 ± 0.04 0.94 ± 0.06 0.98 ± 0.01
Obscuration component 2
NH (1025 m−2) − − − − − 89.5 ± 8.7 94.3 ± 4.4 101.2 ± 9.1 91.2 ± 8.8 78.3 ± 7.4 34.4 ± 1.4
log(ξ) (10−9 W m) − − − − − 0.004 ± 0.1 −3.2 ± 1.1 1.6 ± 0.1 −0.2 ± 0.1 −3.5 ± 0.5 2.1 ± 0.3
Cabs − − − − − 0.42 ± 0.12 0.42 ± 0.06 0.64 ± 0.07 0.20 ± 0.05 0.22 ± 0.04 0.42 ± 0.03
Warm absorbers
log(ξ1) (10−9 W m) 0.59 ± 0.10 0.90 ± 0.12 0.37 ± 0.07 0.07(f) (a) 1.01(f) 0.46 ± 0.05 0.50 ± 0.04 −1.62 ± 0.20 −1.11 ± 0.12 0.08 ± 0.11 −0.48 ± 0.05
log(ξ2) (10−9 W m) 1.93 ± 0.12 1.24 ± 0.07 1.40 ± 0.10 0.01(f) −2.08(f) 1.37 ± 0.11 0.86 ± 0.05 −0.02 ± 0.03 1.35 ± 0.05 1.30 ± 0.17 0.02 ± 0.06
log(ξ3) (10−9 W m) 2.17 ± 0.11 1.86 ± 0.08 2.00 ± 0.06 0.75(f) 0.22(f) 2.53 ± 0.08 1.57 ± 0.08 2.23 ± 0.12 2.88 ± 0.23 2.42 ± 0.07 1.38 ± 0.08
log(ξ4) (10−9 W m) 2.20 ± 0.13 1.89 ± 0.10 1.93 ± 0.05 1.80(f) 1.98(f) 2.25 ± 0.09 2.38 ± 0.07 1.89 ± 0.10 1.92 ± 0.11 1.72 ± 0.45 2.89 ± 0.15
log(ξ5) (10−9 W m) 2.64 ± 0.15 2.23 ± 0.14 2.23 ± 0.09 1.96(f) 2.33(f) 2.35 ± 0.11 2.71 ± 0.08 2.39 ± 0.12 2.49 ± 0.13 2.2 ± 0.5 3.01 ± 0.12
log(ξ6) (10−9 W m) 2.42 ± 0.20 2.70 ± 0.15 2.72 ± 0.10 2.59(f) 2.30(f) 4.03 ± 0.21 2.74 ± 0.09 2.63 ± 0.09 2.67 ± 0.21 3.5 ± 1.5 3.23 ± 0.16
X-ray narrow emission lines 1
NH (1025 m−2) 2.3 ± 0.4 28.1 ± 1.0 18.4 ± 0.9 25.1 ± 2.0 4.8 ± 0.9 7.4 ± 0.5 38.2 ± 0.3 9.3 ± 0.4 3.6 ± 0.3 3.3 ± 0.5 17.9 ± 0.4
log(ξ) (10−9 W m) 0.61 ± 0.05 0.62 ± 0.03 0.82 ± 0.04 −0.16 ± 0.03 0.68 ± 0.2 0.70 ± 0.06 0.27 ± 0.03 0.67 ± 0.04 0.46 ± 0.05 0.46 ± 0.04 0.86 ± 0.05
Cem 0.10 ± 0.02 0.01 ± 0.002 0.01 ± 0.003 0.01 ± 0.01 0.03 ± 0.01 0.04 ± 0.01 0.01 ± 0.01 0.03 ± 0.01 0.04 ± 0.01 0.07 ± 0.02 0.02 ± 0.01
vmic (km s−1) 0 ± 60 700 ± 80 50 ± 50 0 ± 100 0 ± 120 0 ± 70 0 ± 30 440 ± 120 10 ± 210 10 ± 280 90 ± 80
vaver (km s−1) 48 ± 20 240 ± 40 −440 ± 40 1400 ± 80 −700 ± 110 570 ± 90 −220 ± 40 −140 ± 110 −180 ± 190 −140 ± 130 −250 ± 140
X-ray narrow emission lines 2
NH (1025 m−2) 23.8 ± 1.2 − 2.7 ± 0.3 90.9 ± 3.2 − − 8.0 ± 0.4 11.8 ± 0.8 7.3 ± 0.6 1.7 ± 0.2 3.4 ± 0.3
log(ξ) (10−9 W m) 1.52 ± 0.12 − 1.79 ± 0.06 0.51 ± 0.08 − − 1.31 ± 0.07 1.34 ± 0.12 1.33 ± 0.10 1.23 ± 0.07 1.38 ± 0.05
Cem 0.02 ± 0.01 − 0.05 ± 0.01 0.002 ± 0.001 − − 0.02 ± 0.01 0.01 ± 0.01 0.02 ± 0.01 0.05 ± 0.01 0.03 ± 0.01
vmic (km s−1) 500 ± 100 − 0 ± 70 0 ± 110 − − 0 ± 50 520 ± 70 270 ± 120 490 ± 90 740 ± 110
vaver (km s−1) 1990 ± 80 − 1250 ± 100 −460 ± 120 − − 0 ± 40 −240 ± 200 −10 ± 250 20 ± 180 1060 ± 110
X-ray broad emission line
NH (1025 m−2) 0.3 ± 0.1 14.0 ± 0.5 19.3 ± 0.6 28.0 ± 1.9 42.5 ± 4.5 0.9 ± 0.5 5.0 ± 0.4 6.8 ± 0.6 26.8 ± 1.2 29.7 ± 0.9 −
log(ξ) (10−9 W m) −0.3 ± 0.1 1.2 ± 0.1 −0.48 ± 0.12 1.47 ± 0.19 −0.03 ± 0.3 0.12 ± 0.02 1.34 ± 0.04 1.78 ± 0.15 1.35 ± 0.14 1.39 ± 0.09
Cem 0.13 ± 0.02 0.04 ± 0.01 0.06 ± 0.01 0.01 ± 0.01 0.01 ± 0.01 0.01 ± 0.01 0.05 ± 0.01 0.04 ± 0.01 0.05 ± 0.01 0.02 ± 0.01 −
vmac (km s−1) 5700 ± 200 9800 ± 600 4500 ± 700 5100 ± 1100 3200 ± 700 6900 ± 400 9600 ± 500 9700 ± 800 10030 ± 900 8600 ± 1200 −
vaver (km s−1) −1830 ± 500 0 ± 400 −1900 ± 500 40 ± 200 3700 ± 500 −120 ± 190 4000 ± 900 7300 ± 1400 5600 ± 1100 0 ± 300 −
C-stat 1625.37 2144.38 3855.88 1550.82 1379.98 1650.43 2941.37 1711.40 1689.61 1554.50 2223.93
Expected 1363.79 1579.01 3123.64 1367.89 1366.87 1364.10 2130.41 1342.95 1336.58 1357.11 1897.85

Notes.

(a)

These log ξ cannot be well constrained with the current data. They are fixed to the values from Ebrero et al. (2016).

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