Table 2.

Spectral parameters of the X-ray emission of G296.5+10.0.

Parameters#1#2#3#4#5#6#7#8#9#10#11#12
NH (1021)0.83 ± 0.010.84 ± 0.010.81 ± 0.010.82 ± 0.010.85 ± 0.010.74 ± 0.010.81 ± 0.010.79 ± 0.020.83 ± 0.020.82 ± 0.010.82 ± 0.010.77 ± 0.02
kT0.14 ± 0.010.16 ± 0.010.16 ± 0.010.17 ± 0.010.15 ± 0.010.16 ± 0.020.15 ± 0.010.14 ± 0.010.14 ± 0.020.14 ± 0.010.14 ± 0.010.14 ± 0.02
O0.4 ± 0.20.9 ± 0.10.7 ± 0.10.6 ± 0.20.7 ± 0.10.5 ± 0.10.4 ± 0.10.2 ± 0.10.6 ± 0.10.6 ± 0.10.7 ± 0.10.7 ± 0.1
Ne1.2 ± 0.12.2 ± 0.11.6 ± 0.31.7 ± 0.11.9 ± 0.10.7 ± 0.11.2 ± 0.10.5 ± 0.11.8 ± 0.21.5 ± 0.21.7 ± 0.32.3 ± 0.2
Mg1.7 ± 0.71.01.03.3 ± 0.53.8 ± 0.91.01.01.01.01.01.01.0
Fe1.5 ± 0.23.1 ± 0.21.9 ± 0.42.6 ± 0.22.9 ± 0.51.6 ± 0.41.7 ± 0.31.9 ± 0.81.5 ± 0.91.3 ± 0.42.2 ± 0.83.9 ± 0.9
Norm(10−3)8.3 ± 0.28.6 ± 0.33.9 ± 0.28.1 ± 0.29.8 ± 0.13.5 ± 0.18.0 ± 0.27.5 ± 0.29.2 ± 0.38.1 ± 0.24.4 ± 0.28.9 ± 0.2
Flux0 (10−13)39.1 ± 0.474.7 ± 0.836.9 ± 0.7108.7 ± 0.688.5 ± 0.723.1 ± 0.446.3 ± 0.435.6 ± 0.462.2 ± 1.151.8 ± 0.827.2 ± 0.869.3 ± 1.2
|$\chi _\nu ^{2}$|/d.o.f.1.5/5081.6/5241.4/4991.6/5111.5/5131.3/4901.6/4981.3/5751.6/4051.4/5201.1/3991.4/206
EM (1056)1.942.020.911.902.290.821.871.752.151.891.032.08
ne0.190.120.140.140.170.110.190.190.150.140.120.15
Parameters#1#2#3#4#5#6#7#8#9#10#11#12
NH (1021)0.83 ± 0.010.84 ± 0.010.81 ± 0.010.82 ± 0.010.85 ± 0.010.74 ± 0.010.81 ± 0.010.79 ± 0.020.83 ± 0.020.82 ± 0.010.82 ± 0.010.77 ± 0.02
kT0.14 ± 0.010.16 ± 0.010.16 ± 0.010.17 ± 0.010.15 ± 0.010.16 ± 0.020.15 ± 0.010.14 ± 0.010.14 ± 0.020.14 ± 0.010.14 ± 0.010.14 ± 0.02
O0.4 ± 0.20.9 ± 0.10.7 ± 0.10.6 ± 0.20.7 ± 0.10.5 ± 0.10.4 ± 0.10.2 ± 0.10.6 ± 0.10.6 ± 0.10.7 ± 0.10.7 ± 0.1
Ne1.2 ± 0.12.2 ± 0.11.6 ± 0.31.7 ± 0.11.9 ± 0.10.7 ± 0.11.2 ± 0.10.5 ± 0.11.8 ± 0.21.5 ± 0.21.7 ± 0.32.3 ± 0.2
Mg1.7 ± 0.71.01.03.3 ± 0.53.8 ± 0.91.01.01.01.01.01.01.0
Fe1.5 ± 0.23.1 ± 0.21.9 ± 0.42.6 ± 0.22.9 ± 0.51.6 ± 0.41.7 ± 0.31.9 ± 0.81.5 ± 0.91.3 ± 0.42.2 ± 0.83.9 ± 0.9
Norm(10−3)8.3 ± 0.28.6 ± 0.33.9 ± 0.28.1 ± 0.29.8 ± 0.13.5 ± 0.18.0 ± 0.27.5 ± 0.29.2 ± 0.38.1 ± 0.24.4 ± 0.28.9 ± 0.2
Flux0 (10−13)39.1 ± 0.474.7 ± 0.836.9 ± 0.7108.7 ± 0.688.5 ± 0.723.1 ± 0.446.3 ± 0.435.6 ± 0.462.2 ± 1.151.8 ± 0.827.2 ± 0.869.3 ± 1.2
|$\chi _\nu ^{2}$|/d.o.f.1.5/5081.6/5241.4/4991.6/5111.5/5131.3/4901.6/4981.3/5751.6/4051.4/5201.1/3991.4/206
EM (1056)1.942.020.911.902.290.821.871.752.151.891.032.08
ne0.190.120.140.140.170.110.190.190.150.140.120.15

Note. The twelve spectral regions were fitted with a VAPEC model. NH was computed from TBABS XSPEC model in units of cm−2. kT is the electron temperature in units of keV. Norm is the normalization of the fitted models defined as |$10^{-14}/4\pi \, d^2 \times \int n_{\rm H} n_{\rm e}\, {\rm d}V$|⁠, where d is the distance in cm, nH is the hydrogen density in units of cm−3, ne is the electron density in cm−3, and V is the emitting volume in cm3. Flux0 refers to the intrinsic flux in units of |${\rm erg}\, {\rm s}^{-1}\, {\rm cm}^{-2}$|⁠. EM is the emission measure of the X-ray plasma in units of cm−3, defined as |$\int n_{\rm H} n_{\rm e}\, {\rm d}V$|⁠.

Table 2.

Spectral parameters of the X-ray emission of G296.5+10.0.

Parameters#1#2#3#4#5#6#7#8#9#10#11#12
NH (1021)0.83 ± 0.010.84 ± 0.010.81 ± 0.010.82 ± 0.010.85 ± 0.010.74 ± 0.010.81 ± 0.010.79 ± 0.020.83 ± 0.020.82 ± 0.010.82 ± 0.010.77 ± 0.02
kT0.14 ± 0.010.16 ± 0.010.16 ± 0.010.17 ± 0.010.15 ± 0.010.16 ± 0.020.15 ± 0.010.14 ± 0.010.14 ± 0.020.14 ± 0.010.14 ± 0.010.14 ± 0.02
O0.4 ± 0.20.9 ± 0.10.7 ± 0.10.6 ± 0.20.7 ± 0.10.5 ± 0.10.4 ± 0.10.2 ± 0.10.6 ± 0.10.6 ± 0.10.7 ± 0.10.7 ± 0.1
Ne1.2 ± 0.12.2 ± 0.11.6 ± 0.31.7 ± 0.11.9 ± 0.10.7 ± 0.11.2 ± 0.10.5 ± 0.11.8 ± 0.21.5 ± 0.21.7 ± 0.32.3 ± 0.2
Mg1.7 ± 0.71.01.03.3 ± 0.53.8 ± 0.91.01.01.01.01.01.01.0
Fe1.5 ± 0.23.1 ± 0.21.9 ± 0.42.6 ± 0.22.9 ± 0.51.6 ± 0.41.7 ± 0.31.9 ± 0.81.5 ± 0.91.3 ± 0.42.2 ± 0.83.9 ± 0.9
Norm(10−3)8.3 ± 0.28.6 ± 0.33.9 ± 0.28.1 ± 0.29.8 ± 0.13.5 ± 0.18.0 ± 0.27.5 ± 0.29.2 ± 0.38.1 ± 0.24.4 ± 0.28.9 ± 0.2
Flux0 (10−13)39.1 ± 0.474.7 ± 0.836.9 ± 0.7108.7 ± 0.688.5 ± 0.723.1 ± 0.446.3 ± 0.435.6 ± 0.462.2 ± 1.151.8 ± 0.827.2 ± 0.869.3 ± 1.2
|$\chi _\nu ^{2}$|/d.o.f.1.5/5081.6/5241.4/4991.6/5111.5/5131.3/4901.6/4981.3/5751.6/4051.4/5201.1/3991.4/206
EM (1056)1.942.020.911.902.290.821.871.752.151.891.032.08
ne0.190.120.140.140.170.110.190.190.150.140.120.15
Parameters#1#2#3#4#5#6#7#8#9#10#11#12
NH (1021)0.83 ± 0.010.84 ± 0.010.81 ± 0.010.82 ± 0.010.85 ± 0.010.74 ± 0.010.81 ± 0.010.79 ± 0.020.83 ± 0.020.82 ± 0.010.82 ± 0.010.77 ± 0.02
kT0.14 ± 0.010.16 ± 0.010.16 ± 0.010.17 ± 0.010.15 ± 0.010.16 ± 0.020.15 ± 0.010.14 ± 0.010.14 ± 0.020.14 ± 0.010.14 ± 0.010.14 ± 0.02
O0.4 ± 0.20.9 ± 0.10.7 ± 0.10.6 ± 0.20.7 ± 0.10.5 ± 0.10.4 ± 0.10.2 ± 0.10.6 ± 0.10.6 ± 0.10.7 ± 0.10.7 ± 0.1
Ne1.2 ± 0.12.2 ± 0.11.6 ± 0.31.7 ± 0.11.9 ± 0.10.7 ± 0.11.2 ± 0.10.5 ± 0.11.8 ± 0.21.5 ± 0.21.7 ± 0.32.3 ± 0.2
Mg1.7 ± 0.71.01.03.3 ± 0.53.8 ± 0.91.01.01.01.01.01.01.0
Fe1.5 ± 0.23.1 ± 0.21.9 ± 0.42.6 ± 0.22.9 ± 0.51.6 ± 0.41.7 ± 0.31.9 ± 0.81.5 ± 0.91.3 ± 0.42.2 ± 0.83.9 ± 0.9
Norm(10−3)8.3 ± 0.28.6 ± 0.33.9 ± 0.28.1 ± 0.29.8 ± 0.13.5 ± 0.18.0 ± 0.27.5 ± 0.29.2 ± 0.38.1 ± 0.24.4 ± 0.28.9 ± 0.2
Flux0 (10−13)39.1 ± 0.474.7 ± 0.836.9 ± 0.7108.7 ± 0.688.5 ± 0.723.1 ± 0.446.3 ± 0.435.6 ± 0.462.2 ± 1.151.8 ± 0.827.2 ± 0.869.3 ± 1.2
|$\chi _\nu ^{2}$|/d.o.f.1.5/5081.6/5241.4/4991.6/5111.5/5131.3/4901.6/4981.3/5751.6/4051.4/5201.1/3991.4/206
EM (1056)1.942.020.911.902.290.821.871.752.151.891.032.08
ne0.190.120.140.140.170.110.190.190.150.140.120.15

Note. The twelve spectral regions were fitted with a VAPEC model. NH was computed from TBABS XSPEC model in units of cm−2. kT is the electron temperature in units of keV. Norm is the normalization of the fitted models defined as |$10^{-14}/4\pi \, d^2 \times \int n_{\rm H} n_{\rm e}\, {\rm d}V$|⁠, where d is the distance in cm, nH is the hydrogen density in units of cm−3, ne is the electron density in cm−3, and V is the emitting volume in cm3. Flux0 refers to the intrinsic flux in units of |${\rm erg}\, {\rm s}^{-1}\, {\rm cm}^{-2}$|⁠. EM is the emission measure of the X-ray plasma in units of cm−3, defined as |$\int n_{\rm H} n_{\rm e}\, {\rm d}V$|⁠.

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