\begin{table}%t4 %%%%\centering \par \caption{Multi-temperature fitting for {\it XMM} spectra of WR~25. } \begin{tabular}{lll} \hline \hline parameter & rev. \#284 & rev. \#285 \\ \hline $d$ (kpc) assumed & 3.24 & 3.24 \\[+1mm] $N_1^{\rm H}$ (10$^{21}$~cm$^{-2}$) & $7.7\pm0.6$ & $6.3\pm0.6$ \\[+1mm] $N_2^{\rm H}$ (10$^{21}$~cm$^{-2}$) & $2.4\pm0.7$ & $3.2\pm0.6$ \\[+1mm] $T_1$ (MK) & $7.1\pm0.3$ & $6.9\pm0.3$ \\[+1mm] $T_2$ (MK) & $33\pm4$ & $30\pm 2$ \\[+1mm] $EM_1$ (10$^{56}$~cm$^{-3}$) & $7.4\pm1.1$ & $6.1\pm0.9$ \\[+1mm] $EM_2$ (10$^{56}$~cm$^{-3}$) & $3.0\pm0.5$ & $2.6\pm0.2$ \\[+1mm] %$L_{\rm x}$ [0.1~-~10~keV] (10$^{32}$~erg~s$^{-1}$) & 185$\pm$21 & 180$\pm$17 \\[+1mm] $L_{\rm x}$ [0.5--10~keV] (10$^{32}$~erg~s$^{-1}$) & $128\pm14$ & $129\pm 12$ \\[+1mm] % & & \\[-2mm] Abundances$^a$: & & \\[+1mm] He & 2.27$^b$ & 2.27$^b$ \\[+1mm] C & 0.15$^b$ & 0.15$^b$ \\[+1mm] N & 5.9$^b$ & 5.9$^b$ \\[+1mm] O & $<$0.4 & $<$0.24 \\[+1mm] Ne & 0.54$^{+0.15}_{-0.15}$ & 0.48$^{+0.11}_{-0.11}$ \\[+1mm] Mg & 0.67$^{+0.09}_{-0.09}$ & 0.58$^{+0.08}_{-0.08}$ \\[+1mm] Si & 0.83$^{+0.10}_{-0.10}$ & 0.86$^{+0.10}_{-0.10}$ \\[+1mm] S & 1.3$^{+0.2}_{-0.2}$ & 1.1$^{+0.2}_{-0.2}$ \\[+1mm] Fe$_1$ & 0.56$^{+0.05}_{-0.05}$ & 0.40$^{+0.03}_{-0.03}$ \\[+1mm] Fe$_2$ & 0.64$^{+0.14}_{-0.14}$ & 0.62$^{+0.10}_{-0.10}$ \\[+1mm] % & & \\[-2mm] % & & \\[-2mm] \gired & 643/619 & 727/613 \\ \hline \par \end{tabular} \begin{flushleft} { \begin{description} \item Notes: \item $L_{\rm x}$ values unabsorbed i.e., corrected for absorption by the ISM and stellar wind. \item $^a$ Relative to solar photospheric number abundances (Anders \& Grevesse \cite{Anders89} or Grevesse \& Sauval \cite{Grevesse98} and 1999 for Fe). \item $^b$ Fixed on literature values given in Sect.~3.2.2. \end{description} } \end{flushleft} \end{table}