\begin{table}%T2 \par \caption{\label{datos_fir}\FIR\ and \FUV\ data for the WR~galaxy sample analyzed in this work. } \small%\centering \par \begin{tabular}{l cccc c c cc} \hline\hline\noalign{\smallskip} Galaxy & $f_{\rm 12~\mu m}$ & $f_{\rm 25~\mu m}$ & $f_{\rm 60~\mu m}$ & $f_{\rm 100~\mu m}$ & $F_{\rm FIR}$ & Reg. & $m_{\rm FUV}$ & $f_{\rm FUV}$ \\ & [Jy] & [Jy] & [Jy] & [Jy] & \tablefootmark{a} & \tablefootmark{b} &[mag] & \tablefootmark{c} \\ \hline HCG 31 & 0.110~$\pm$~0.020 & 0.580~$\pm$~0.040 & 3.92~$\pm$~0.31 & 5.84~$\pm$~0.47 & 2.01~$\pm$~0.16 &AC&14.97~$\pm$~0.06 & 7.54~$\pm$~0.44\\ & & & & & &B& 16.80~$\pm$~0.09 & 3.32~$\pm$~0.26\\ & & & & & &E& 18.01~$\pm$~0.08 & 0.456~$\pm$~0.035\\ & & & & & &F& 18.24~$\pm$~0.11 & 0.460~$\pm$~0.047\\ & & & & & &G& 15.93~$\pm$~0.06 & 3.11~$\pm$~0.18\\ & & & & & &H& 20.63~$\pm$~0.40 & 0.0041~$\pm$~0.0014\\ Mkn 1087 & 0.103~$\pm$~0.029 & 0.414~$\pm$~0.058 & 3.03~$\pm$~0.33 & 4.44~$\pm$~0.40 & 1.54~$\pm$~0.16 &\nodata& \nodata&\nodata \\ Haro 15 & 0.118~$\pm$~0.034 & 0.297~$\pm$~0.089 & 1.36~$\pm$~0.12 & 1.97~$\pm$~0.20 & 0.690~$\pm$~0.064&\nodata& 15.12~$\pm$~0.07& 9.41~$\pm$~0.57\\ Mkn 1199 & 0.282~$\pm$~0.031 & 1.28~$\pm$~0.09 & 6.82~$\pm$~0.34 & 8.85~$\pm$~0.53 & 3.33~$\pm$~0.18 &\nodata& \nodata&\nodata \\ Mkn 5 & $<$0.0503 & $<$0.0533 & 0.21~$\pm$~0.04 & $<$0.8473 & $<$1.75 &\nodata& 17.76~$\pm$~0.07 & 1.59~$\pm$~0.10\\ IRAS 08208+2816& 0.126~$\pm$~0.029 & 0.278~$\pm$~0.067 & 1.15~$\pm$~0.09 & 1.70~$\pm$~0.17 & 0.588~$\pm$~0.051&\nodata& 16.59~$\pm$~0.07 & 3.75~$\pm$~0.23\\ IRAS 08339+6517& 0.250~$\pm$~0.025 & 1.13~$\pm$~0.02 & 5.81~$\pm$~0.04 & 6.48~$\pm$~0.09 & 2.71~$\pm$~0.02 & & 15.37~$\pm$~0.06 & 10.7~$\pm$~0.6\\ & & & & & &c& 19.70~$\pm$~0.10 & 0.160~$\pm$~0.014\\ POX 4 & $<$0.987 & 0.153~$\pm$~0.040 & 0.629~$\pm$~0.057 & $<$0.5798 & $<$0.278 &POX~4& 16.03~$\pm$~0.06 & 2.82~$\pm$~0.16\\ & & & & & &Comp.& 19.06~$\pm$~0.12 & 0.269~$\pm$~0.030 \\ UM 420 & \nodata & $<$0.275 & 0.411: & 0.613: & 0.211: &\nodata& 18.22~$\pm$~0.06 & 0.377~$\pm$~0.021\\ SBS 0926+606 & $<$0.07553 & $<$0.08818 & 0.269~$\pm$~0.046 & $<$0.5296 & $<$0.154 &A& 16.71~$\pm$~0.06 & 1.75~$\pm$~0.09\\ & & & & & &B& 17.84~$\pm$~0.10 & 0.829~$\pm$~0.073\\ SBS 0948+532 & \nodata & \nodata& \nodata & \nodata & \nodata &\nodata& \nodata&\nodata \\ SBS 1054+365 & $<$0.055 & $<$0.100 & 0.536~$\pm$~0.048 & 0.97~$\pm$~0.15 & 0.296~$\pm$~0.035&\nodata& 16.67~$\pm$~0.07 & 1.18~$\pm$~0.08 \\ SBS 1211+540 & \nodata & \nodata& \nodata & \nodata & \nodata &\nodata& 18.40~$\pm$~0.07 & 0.370~$\pm$~0.022\\ SBS 1319+579 & \nodata & \nodata& 0.209: & 0.685: & 0.154: &\nodata& 17.00~$\pm$~0.06 & 0.864~$\pm$~0.048\\ & & & & & & A & 18.60~$\pm$~0.06 & 0.199~$\pm$~0.010\\ SBS 1415+437 & \nodata & \nodata& \nodata & \nodata & \nodata &\nodata& 16.22~$\pm$~0.06 & 3.95~$\pm$~0.22\\ III Zw 107 & $<$0.0968 & 0.336~$\pm$~0.050 & 1.37~$\pm$~0.20 & 1.72~$\pm$~0.31& 0.662~$\pm$~0.104&\nodata& \nodata&\nodata\\ Tol 9 & 0.111~$\pm$~0.030 & 0.465~$\pm$~0.051 & 2.71~$\pm$~0.22 & $<$5.516 & $<$1.58 &\nodata& 17.57~$\pm$~0.07& 4.22~$\pm$~0.22\\ Tol 1457-262 & $<$0.117 & 0.611~$\pm$~0.067 & 3.09~$\pm$~0.19 & 3.68~$\pm$~0.40& 1.47~$\pm$~0.11 &\nodata& 15.84~$\pm$~0.07& 6.95~$\pm$~0.47\\ & & & & & &Obj~1& 16.15~$\pm$~0.06 & 5.26~$\pm$~0.29\\ & & & & & &Obj~2& 17.41~$\pm$~0.13 & 1.64~$\pm$~0.18\\ & & & & & &\#15& 19.71~$\pm$~0.21 & 0.199~$\pm$~0.037\\ Arp 252 & 0.188~$\pm$~0.023 & 0.994~$\pm$~0.050 & 3.91~$\pm$~0.20 & 4.11~$\pm$~0.25& 1.79~$\pm$~0.10 &A& 18.67~$\pm$~0.08 & 1.91~$\pm$~0.13\\ & & & & & &B& 18.84~$\pm$~0.07 & 0.441~$\pm$~0.027\\ NGC 5253 & 2.50~$\pm$~0.02 & 12.07~$\pm$~0.05 & 29.84~$\pm$~0.07 &30.08~$\pm$~0.21& 13.49~$\pm$~0.05 &\nodata& 12.81~$\pm$~0.06 & 123.0~$\pm$~6.5\\ \hline \end{tabular} \tablefoot{\tablefoottext{a}{In units of $10^{-10}$ erg s$^{-1}$ cm$^{-2}$.}\\ \tablefoottext{b}{Region within each system (HCG~31, IRAS~08339+6517, POX~4, SBS~0926+606, SBS~1319+579, Tol~1457-262, and Arp~252; see Paper~I). }\\ \tablefoottext{c}{In units of $10^{-14}$ erg s$^{-1}$ cm$^{-2}$ \AA$^{-1}$. } } \vspace*{4mm} \end{table}