Spatially resolved XMM-Newton analysis and a model of the nonthermal emission of MSH 15–52

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Table 3:

Results obtained by fitting a power-law spectrum to the XMM-Newton data of MSH 15-52.
Ring	$\Gamma$	Flux	Surface Brightness	$\chi^{2}/{\rm d.o.f.}$
No.		(10^-12 erg cm^-2 s^-1)	(10^-17 erg cm^-2 s^-1 $~{\rm arcsec}^{-2}$ )
1	$1.66 \pm 0.02$	$12.0 \pm 0.3$	$162 \pm 4.5$	147/161
2	$1.78 \pm 0.03$	$10.0 \pm 0.3$	$92 \pm 3.0$	161/147
3	$1.88 \pm 0.02$	$2.9 \pm 0.07$	$9.2 \pm 0.2$	431/459
4	$1.96 \pm 0.02$	$3.1 \pm 0.09$	$6.1 \pm 0.2$	356/536
5	$2.07 \pm 0.05$	$2.4 \pm 0.1$	$3.4 \pm 0.2$	97/156
6	$2.24 \pm 0.28$	$0.4 \pm 0.2$	$0.5 \pm 0.3$	62/107

Source LaTeX | All tables | In the text

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