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Table 2:

The best-fit NEI parameters of the XMM-Newton EPIC, RGS and Chandra ACIS data.

Parameter
RGS EPIC MOS + ACIS ACIS inner ACIS outer

$n_{\rm e}n_{\rm H}~V\; (10^{58},\;{\rm cm}^{-3}$)
$1.8^{+2.5}_{\rm -1.8}$ $3.7_{\rm -0.2}^{+0.2}$ $2.63_{\rm -0.32}^{+0.33}$ $0.66_{\rm -0.08}^{+6.49}$
$kT_{\rm e}$ (keV) $2.21^{+0.08}_{\rm -0.07}$ $2.82_{\rm -0.03}^{+0.03}$ $2.88_{\rm -0.06}^{+0.06}$ $1.73_{\rm -1.07}^{+0.14}$
$n_{\rm e}t\; (10^{10},\;{\rm s\;cm}^{-3})$ $2.69^{+0.03}_{\rm -0.03}$ $2.27_{\rm -0.01}^{+0.01}$ $2.22_{\rm -0.002}^{+0.02}$ $3.90 \pm N/A$
$n_{\rm H}\; (10^{21},\;{\rm cm}^{-2}$) - $2.62_{\rm -0.06}^{+0.07}$ $2.74_{\rm -0.11}^{+0.11}$ -

$\chi^2$/d.o.f.
2.4 29.4 10.4 2.5

Notes. Columns 1 and 2 list data for the entire remnant. Column 3 lists data for the inner shell of the SNR and Col. 4 - for the outer shell (see Fig. 7).


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