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Table A.2

Additional results and physical properties.

Physical propertiesa RGS-band 2σ limitsb Emission-line 2σ limitsc 2-T 2σ limitsd
Source d(Mpc) kpc/1′′ r500 K0 T cS M aREQ v vSC Ma M aSC O viii Fe xvii Fe xx+ v1 v2
2A0335+096 149 0.72 1.05 7.1 1.6 640 0.27 880 400 1.37 0.63 580 – 530 – –
A 85 238 1.15 1.21 12.5 2.3 780 0.28 910 360 1.16 0.46 480 – 570 – –
A 133 243 1.18 0.94 17.3 4.5 1090 0.13 1050 410 0.96 0.37 460 – 603 – –
A 189 137 0.66 0.50 4.0 0.9 500 0.18 950 450 1.91 0.90 650 – 3010 – –
A 262 69 0.34 0.74 10.6 1.7 670 0.17 300 180 0.45 0.27 510 – 790 – –
A 496 140 0.68 1.00 8.9 2.8 870 0.18 1520 710 1.75 0.82 480 – 710 – –
A 1795 264 1.28 1.22 19.0 1.8 690 0.36 2300 870 3.35 1.27 930 – 1750 – –
A 1991 251 1.22 0.82 1.5 2.7 840 0.21 520 200 0.62 0.24 630 – 900 – –
A 2029 328 1.59 1.33 10.5 2.6 840 0.23 500 180 0.60 0.21 810 – 2310 – –
A 2052 149 0.72 0.95 9.5 3.2 920 0.21 910 420 0.99 0.45 600 – 690 – –
A 2199 129 0.63 1.00 13.3 1.3 590 0.28 560 270 0.95 0.46 540 – 1010 – –
A 2597 365 1.77 1.11 10.6 2.6 840 0.23 1300 440 1.55 0.53 500 – 990 – –
A 2626 245 1.19 0.84 23.2 1.3 600 0.23 2300 890 3.85 1.49 – – – – –
A 3112 315 1.53 1.13 11.4 1.4 600 0.25 1390 500 2.30 0.82 500 – 570 – –
A 3526 44 0.21 0.83 2.3 2.3 790 0.20 400 280 0.51 0.35 390 230 730 530 240
A 3581 91 0.44 0.72 9.5 2.7 850 0.14 960 520 1.13 0.61 1150 – 1060 – –
A 4038 128 0.62 0.89 37.9 2.3 790 0.18 3200 1540 4.06 1.96 1540 – 5290 – –
A 4059 215 1.04 0.96 7.1 3.2 920 0.19 1730 700 1.88 0.76 1090 – 1120 – –
AS 1101 248 1.20 0.98 10.4 2.4 800 0.23 910 350 1.15 0.44 530 – 690 – –
AWM 7 73 0.35 0.86 8.4 1.9 700 0.22 600 350 0.85 0.50 1650 – – – –
EXO 0422 167 0.81 0.89 13.8 2.4 800 0.18 1400 620 1.75 0.77 1140 – 1170 – –
Fornax 19 0.09 0.40 2.6 1.0 520 0.16 260 240 0.50 0.46 390 300 520 – –
HCG 62 60 0.29 0.46 3.4 0.8 480 0.23 560 350 1.18 0.73 910 320 1350 2370 260
Hydra-A 222 1.08 1.07 13.3 3.4 950 0.21 1050 420 1.10 0.44 700 – 1050 – –
M 49 17.1 0.08 0.53 0.9 0.9 490 0.17 320 300 0.65 0.62 520 340 940 1050 240
M 86 16 0.08 0.49 8.0 0.8 450 0.22 660 640 1.46 1.41 – – – – –
M 87 16.4 0.08 0.75 3.5 1.4 600 0.25 470 450 0.78 0.75 400 – 430 – –
M 89 15.3 0.07 0.44 3.0 0.6 400 0.20 670 660 1.67 1.63 1330 960 1430 – –
MKW 3s 192 0.93 0.95 23.9 2.7 840 0.16 680 290 0.81 0.34 720 – 1310 – –
MKW 4 80 0.39 0.62 6.9 1.5 630 0.31 620 350 0.99 0.56 660 – 700 – –
NGC 507 65.5 0.32 0.60 1.0 0.7 420 0.22 5000 3010 11.87 7.15 4210 1310 4560 6540 1680
NGC 1316 19 0.09 0.46 1.0 0.7 420 0.20 240 220 0.57 0.52 410 250 4780 – –
NGC 1404 20 0.10 0.61 5.5 1.2 560 0.23 650 580 1.16 1.04 1020 690 1180 – –
NGC 1550 53.6 0.26 0.62 6.6 0.9 500 0.22 1250 800 2.49 1.60 860 – 1010 – –
NGC 3411 66.3 0.32 0.47 3.7 0.7 440 0.21 720 430 1.65 0.99 1790 1520 1570 – –
NGC 4261 29.4 0.14 0.45 3.0 0.9 500 0.19 230 180 0.47 0.37 650 290 620 – –
NGC 4325 108 0.52 0.58 4.7 0.7 420 0.29 680 350 1.63 0.83 1690 540 1870 – –
NGC 4374 18.4 0.09 0.46 8.0 0.7 420 0.19 280 260 0.66 0.61 510 550 900 – –
NGC 4636 14.3 0.07 0.35 1.4 0.9 480 0.13 300 300 0.62 0.62 310 290 1410 – –
NGC 4649 17.3 0.08 0.53 4.6 0.9 490 0.19 390 370 0.80 0.75 370 580 590 – –
NGC 5044 38.9 0.19 0.56 2.3 1.1 540 0.24 400 290 0.74 0.53 500 350 1770 790 280
NGC 5813 29.7 0.14 0.44 1.4 0.7 430 0.24 160 130 0.37 0.29 470 170 1690 – –
NGC 5846 26.3 0.13 0.36 1.8 0.7 430 0.39 190 160 0.44 0.36 320 190 1470 300 180
Perseus 73.6 0.36 1.29 19.4 2.8 860 0.28 1600 926 1.86 1.08 1160 – 1670 – –

Notes.

(a)

r500 (in Mpc units) and K0 (in keV cm-2 units) were taken from the ACCEPT catalog (Cavagnolo et al. 2009) with the exceptions of M 86 (Finoguenov et al. 2004), NGC 1316 (Tashiro et al. 2006), NGC 4649, and NGC 4261 (Werner et al. 2012), A 189, Fornax, HCG 62, M 49, NGC 1550, NGC 3411, NGC 4325, NGC 4636, NGC 5044, NGC 5813, and NGC 5846 (Panagoulia et al. 2014a). NGC 4374 and NGC 1404 profiles were calculated following the method of Werner et al. (2012). The temperatures (in keV units) are estimated with the 0.8′ region RGS best-fit isothermal model, and they are used to compute the sound speed, cS, which is reported in units of km s-1 (see Sect. 5.2). MaREQ is the Mach number which is required to make a heating–cooling balance. It is calculated with Eq. (2) in Sect. 5.2.

(b)

90% limits on velocity and Mach number for the 0.8′ region, obtained by subtracting the best-fit spatial line broadening, and 90% limits normalized by the physical scale, assuming Kolmogorov turbulence (see Sects. 4.2 and 5.2; Figs. 3 and A.3; and last column in Table A.1).

(c)

90% velocity limits separately measured for the relevant emission lines with an isothermal cluster model (see Sect. 5.1).

(d)

90% velocity limits separately measured for the two CIE components with the multi-temperature cluster model (see Sect. 5.1).

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