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Table 4

Wolf–Rayet abundances model: tbabs× vphabs× ∑ vapec.

Name NH (1022 cm−2) kT (keV) Norm χν2$\[\chi_\nu^2\]$ or Prob (χ2/dof) FX[ FXISMcor]$\[\mathrm{F}_X\left[\mathrm{~F}_{\mathrm{X}}^{\mathrm{ISMcor}}\right]\]$ (erg cm−2 s−1) LX[ LXISMcor ]$\[\mathrm{L}_X\left[\mathrm{~L}_{\mathrm{X}}^{\text {ISMcor }}\right]\]$ (erg s−1)
WN abundances with He/H=100 solar
A (9.71−0.64+0.71$\[9.71_{-0.64}^{+0.71}\]$)e−2 0.11±0.01 (0.64−0.42+1.96$\[0.64_{-0.42}^{+1.96}\]$) 1.04(294.3/282) (1.66−0.06+0.01$\[1.66_{-0.06}^{+0.01}\]$[2.43])e−13 (3.56−0.14+0.02$\[3.56_{-0.14}^{+0.02}\]$[5.2])e32
0.83−0.05+0.04$\[0.83_{-0.05}^{+0.04}\]$ (5.35−0.82+1.17$\[5.35_{-0.82}^{+1.17}\]$)e−5
6.0−1.4+1.5$\[6.0_{-1.4}^{+1.5}\]$ (2.54−0.31+0.52$\[2.54_{-0.31}^{+0.52}\]$)e−6
B (a) (3.52−0.55+0.61$\[3.52_{-0.55}^{+0.61}\]$)e−2 0.84±0.15 (2.78−0.67+1.13$\[2.78_{-0.67}^{+1.13}\]$)e−6 1.13(164.38/145) (5.93−0.24+0.07$\[5.93_{-0.24}^{+0.07}\]$)e−14 (1.27−0.05+0.02$\[1.27_{-0.05}^{+0.02}\]$[1.73])e32
4.55−0.82+1.16$\[4.55_{-0.82}^{+1.16}\]$ (1.8−0.27+0.31$\[1.8_{-0.27}^{+0.31}\]$)e−6
U (b) (2.29−0.58+0.78$\[2.29_{-0.58}^{+0.78}\]$)e−2 0.6−0.14+0.17$\[0.6_{-0.14}^{+0.17}\]$ (2.7−1.0+2.9$\[2.7_{-1.0}^{+2.9}\]$)e−6 1.13(110.71/98) (3.06−0.24+0.02$\[3.06_{-0.24}^{+0.02}\]$[5.66])e−14 (6.55−0.52+0.05$\[6.55_{-0.52}^{+0.05}\]$[12.12])e31
2.16−0.32+0.45$\[2.16_{-0.32}^{+0.45}\]$ (1.36−0.34+0.41$\[1.36_{-0.34}^{+0.41}\]$)e−6
L (c) (6.2−3.2+3.1$\[6.2_{-3.2}^{+3.1}\]$)e−2 0.26−0.08+0.39$\[0.26_{-0.08}^{+0.39}\]$ (0.43−0.42+8.7$\[0.43_{-0.42}^{+8.7}\]$)e−4 0.89(58.86/66) (2.16−0.36+0.01$\[2.16_{-0.36}^{+0.01}\]$[3.04])e−14 (4.63−0.77+0.02$\[4.63_{-0.77}^{+0.02}\]$[6.51])e31
2.06−0.41+0.8$\[2.06_{-0.41}^{+0.8}\]$ (1.66−0.65+0.87$\[1.66_{-0.65}^{+0.87}\]$)e−6
O (d) (1.05−0.92+1.6$\[1.05_{-0.92}^{+1.6}\]$)e−2 0.63−0.2+0.28$\[0.63_{-0.2}^{+0.28}\]$ (2.7−1.7+10.0$\[2.7_{-1.7}^{+10.0}\]$)e−7 1.1(22.05/20) (1.03−0.9+0.04$\[1.03_{-0.9}^{+0.04}\]$[1.71])e−14 (2.2−1.92+0.08$\[2.2_{-1.92}^{+0.08}\]$[3.66])e31
>9.9 (2.09−0.37+0.44$\[2.09_{-0.37}^{+0.44}\]$)e−7
*W (3.4−1.2+2.5$\[3.4_{-1.2}^{+2.5}\]$)e−1 0.25−0.09+0.11$\[0.25_{-0.09}^{+0.11}\]$ (2.2−2.1+47.7$\[2.2_{-2.1}^{+47.7}\]$)e−3 0.31(46.93/43) (1.0−0.66+0.01$\[1.0_{-0.66}^{+0.01}\]$[1.09])e−14 (2.14−1.41+0.02$\[2.14_{-1.41}^{+0.02}\]$[2.34])e31
4.2−2.4+3.6$\[4.2_{-2.4}^{+3.6}\]$ (7.9−2.9+17.3$\[7.9_{-2.9}^{+17.3}\]$)e−7
*J (9.3−5.2+14.7$\[9.3_{-5.2}^{+14.7}\]$)e−2 0.18−0.16+0.53$\[0.18_{-0.16}^{+0.53}\]$ (8.8−8.8+370.6$\[8.8_{-8.8}^{+370.6}\]$)e−5 0.07(57.48/43) (6.78−3.47+0.10$\[6.78_{-3.47}^{+0.10}\]$[7.79])e−15 (1.45−0.74+0.02$\[1.45_{-0.74}^{+0.02}\]$[1.67])e31
5.13−3.12+7.01$\[5.13_{-3.12}^{+7.01}\]$ (0.03−0.01+0.1$\[0.03_{-0.01}^{+0.1}\]$)e−5
*R (e) (3.1−1.1+1.7$\[3.1_{-1.1}^{+1.7}\]$)e−1 0.24−0.1+0.12$\[0.24_{-0.1}^{+0.12}\]$ (2.6−2.6+43.5$\[2.6_{-2.6}^{+43.5}\]$)e−3 0.61(33.01/36) (5.91−4.56+0.10$\[5.91_{-4.56}^{+0.10}\]$[6.66])e−15 (1.27−0.98+0.02$\[1.27_{-0.98}^{+0.02}\]$[1.43])e31
3.9−1.8+2.9$\[3.9_{-1.8}^{+2.9}\]$ (4.7−1.7+8.6$\[4.7_{-1.7}^{+8.6}\]$)e−7
*X (8.59−3.32+4.48$\[8.59_{-3.32}^{+4.48}\]$)e−2 >3.38 (2.35−0.57+1.49$\[2.35_{-0.57}^{+1.49}\]$)e−7 0.79(23.5/30) (5.68−2.25+0.16$\[5.68_{-2.25}^{+0.16}\]$[6.28])e−15 (12.16−4.83+0.35$\[12.16_{-4.83}^{+0.35}\]$[13.44])e30
*G (f) 44 3.96−0.93+1.79$\[3.96_{-0.93}^{+1.79}\]$ (9.4±2.5)e−7 0.02(48.63/30) (6.52−1.13+0.41$\[6.52_{-1.13}^{+0.41}\]$[8.16])e−15 (1.39−0.24+0.09$\[1.39_{-0.24}^{+0.09}\]$[1.74])e31
*P (4.5−1.6+3.2$\[4.5_{-1.6}^{+3.2}\]$)e−1 4.6−2.8+4.6$\[4.6_{-2.8}^{+4.6}\]$ (4.5−1.9+19.8$\[4.5_{-1.9}^{+19.8}\]$)e−7 0.16(22.8/17) (4.79−3.98+0.05$\[4.79_{-3.98}^{+0.05}\]$[5.01])e−15 (10.25−8.53+0.11$\[10.25_{-8.53}^{+0.11}\]$[10.72])e30
*I (5.1−1.7+2.0$\[5.1_{-1.7}^{+2.0}\]$)e−1 0.11−0.04+0.05$\[0.11_{-0.04}^{+0.05}\]$ (3.0−3.0+55$\[3.0_{-3.0}^{+55}\]$)e2 0.16(19.25/14) (3.64−3.43+0.01$\[3.64_{-3.43}^{+0.01}\]$[3.88])e−15 (7.79−7.35+0.02$\[7.79_{-7.35}^{+0.02}\]$[8.32])e30
4.9−2.6+7.0$\[4.9_{-2.6}^{+7.0}\]$ (3.5−1.5+3.3$\[3.5_{-1.5}^{+3.3}\]$)e−7
*Q (1.12−0.43+0.75$\[1.12_{-0.43}^{+0.75}\]$)e−1 >3.1 (1.75−0.49+1.79$\[1.75_{-0.49}^{+1.79}\]$)e−7 0.3(17.29/15) (3.93−2.17+0.15$\[3.93_{-2.17}^{+0.15}\]$[4.29])e−15 (8.41−4.64+0.33$\[8.41_{-4.64}^{+0.33}\]$[9.18])e30
*D (9.9−6.6+4.4$\[9.9_{-6.6}^{+4.4}\]$)e−1 >1.0 (5.3−5.3+14.5$\[5.3_{-5.3}^{+14.5}\]$)e−6 0.71(10.74/14) (2.76−2.76+0.01$\[2.76_{-2.76}^{+0.01}\]$[2.89])e−15 (5.91−5.91+0.02$\[5.91_{-5.91}^{+0.02}\]$[6.18])e30
*V 1.39−0.41+0.67$\[1.39_{-0.41}^{+0.67}\]$ 0.1 (3.8−3.8+148.5$\[3.8_{-3.8}^{+148.5}\]$)e6 0.58(10.39/12) (5.12−5.12+0.01$\[5.12_{-5.12}^{+0.01}\]$[5.35])e−15 (10.96−10.96+0.02$\[10.96_{-10.96}^{+0.02}\]$[11.45])e30
1.78−0.63+5.35$\[1.78_{-0.63}^{+5.35}\]$ (5.8−5.1+39.3$\[5.8_{-5.1}^{+39.3}\]$)e−6
*S (6.1−6.1+10.1$\[6.1_{-6.1}^{+10.1}\]$)e−2 1.35−0.74+3.61$\[1.35_{-0.74}^{+3.61}\]$ (8.1−8.1+93.9$\[8.1_{-8.1}^{+93.9}\]$)e−8 0.83(1.47/4) (4.84−4.84+0.05$\[4.84_{-4.84}^{+0.05}\]$[6.74])e−16 (1.04−1.04+0.01$\[1.04_{-1.04}^{+0.01}\]$[1.44])e30
WC abundances with He/H=100 solar
F (g) (3.7−1.1+1.2$\[3.7_{-1.1}^{+1.2}\]$)e−3 0.06−0.02+0.03$\[0.06_{-0.02}^{+0.03}\]$ 2.5−2.5+4563.2$\[2.5_{-2.5}^{+4563.2}\]$ 1.03(49.66/48) (3.28−0.67+0.01$\[3.28_{-0.67}^{+0.01}\]$[3.82])e−14 (7.03−1.43+0.02$\[7.03_{-1.43}^{+0.02}\]$[8.19])e31
0.7−0.25+0.34$\[0.7_{-0.25}^{+0.34}\]$ (2.9−2.1+13.1$\[2.9_{-2.1}^{+13.1}\]$)e−7
5.6−1.4+2.6$\[5.6_{-1.4}^{+2.6}\]$ (1.17−0.17+0.23$\[1.17_{-0.17}^{+0.23}\]$)e−7
*N (8.3±1.9)e−3 0.08−0.02+0.08$\[0.08_{-0.02}^{+0.08}\]$ 4.9−4.8+433.4$\[4.9_{-4.8}^{+433.4}\]$) 0.24(72.87/65) (1.42−0.24+0.03$\[1.42_{-0.24}^{+0.03}\]$[1.55])e−14 (3.03−0.5+0.06$\[3.03_{-0.5}^{+0.06}\]$[3.32])e31
1.61−0.23+0.21$\[1.61_{-0.23}^{+0.21}\]$ (2.47−0.93+1.38$\[2.47_{-0.93}^{+1.38}\]$)e−7
*E (0.29−0.29+70868.82$\[0.29_{-0.29}^{+70868.82}\]$)e−8 2.9−1.4+3.2$\[2.9_{-1.4}^{+3.2}\]$ (6.4−1.4+4.5$\[6.4_{-1.4}^{+4.5}\]$)e−9 0.62(8.14/10) (1.49−0.56+0.14$\[1.49_{-0.56}^{+0.14}\]$[3.14])e−15 (3.2−1.19+0.31$\[3.2_{-1.19}^{+0.31}\]$[6.73])e30
*H (1.77−0.81+1.07$\[1.77_{-0.81}^{+1.07}\]$)e−3 0.28 (12.8−8.5+22.9$\[12.8_{-8.5}^{+22.9}\]$)e−8 0.08(12.88/7) (3.13−1.22+0.59$\[3.13_{-1.22}^{+0.59}\]$[7.2])e−16 (6.7−2.6+1.2$\[6.7_{-2.6}^{+1.2}\]$[15.4])e29

Notes. Same as in Table 3. Abundances of specific elements that were varied relative to that of helium (for reference, the generic values are reported in Sec. 3.5)(a) S:126−36+46$\[\text{S:} 126_{-36}^{+46}\]$ (b)S=96.1±31.0(c)S=85.09±38.0 (d)S=829, Ar=1000. (e)A Gaussian line was added in the model at 5.21 keV (see Notes in Table 3). (f) A model of the form tbabs× pcfabs× ∑vapec was used in this particular case with the parameter for the covering fraction frozen at 0.95. (g)Si=2930, Ar=3100, Ca=8173, Fe=460.

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