\begin{table}%t6 \caption{\label{12745tb6}Supernovae type Ia fraction, $f = {\rm SNIa}/({\rm SNIa+SNcc})$, obtained for different theoretical SNe models from the observed Si/Fe and Ni/Fe abundance ratios. SNIa and SNcc models are the same as in Table~\ref{12745tb5}.} \small%\centering \par \begin{tabular}{r| c c c c c c c} \hline\hline {\it mekal} model & & & & SNIa & & &\\ \hline SNcc & W7 & W70 & WDD1 & WDD2 & WDD3 & CDD1 & CDD2 \\ \hline No06,S &$0.117{-}0.136$&$0.110{-}0.244$&$ $&$ $&$ $&$ $&$ $\\ No06,T &$0.139{-}0.141$&$0.132{-}0.272$&$ $&$ $&$ $&$ $&$ $\\ CL04,S &$ $&$0.149{-}0.193$&$ $&$0.168{-}0.384$&$0.134{-}0.289$&$ $&$0.154{-}0.348$\\ CL04,T &$ $&$0.182{-}0.320$&$ $&$0.204{-}0.313$&$0.165{-}0.327$&$ $&$0.188{-}0.302$\\ W95,S &$ $&$ $&$0.207{-}0.254$&$0.129{-}0.322$&$0.102{-}0.237$&$0.226{-}0.239$&$0.118{-}0.289$\\ W95,T &$ $&$ $&$ $&$0.143{-}0.338$&$0.113{-}0.250$&$ $&$0.131{-}0.304$\\ \hline \noalign{\medskip} \noalign{\medskip} \hline\hline {\it apec} model & & & & SNIa & & &\\ \hline SNcc & W7 & W70 & WDD1 & WDD2 & WDD3 & CDD1 & CDD2 \\ \hline No06,S &$ $&$0.096{-}0.109$&$ $&$0.107{-}0.270$&$0.086{-}0.200$&$ $&$0.098{-}0.243$\\ No06,T &$ $&$ $&$ $&$0.130{-}0.301$&$0.104{-}0.225$&$ $&$0.119{-}0.272$\\ CL04,S &$ $&$ $&$0.221{-}0.606$&$0.144{-}0.345$&$0.174{-}0.262$&$0.239{-}0.517$&$0.133{-}0.313$\\ CL04,T &$ $&$ $&$0.269{-}0.543$&$0.179{-}0.388$&$0.145{-}0.300$&$0.290{-}0.453$&$0.166{-}0.354$\\ W95,S &$ $&$ $&$0.172{-}0.556$&$0.197{-}0.286$&$ $&$0.186{-}0.564$&$0.189{-}0.258$\\ W95,T &$ $&$ $&$0.191{-}0.574$&$0.147{-}0.301$&$ $&$0.207{-}0.517$&$0.141{-}0.272$\\ \hline \end{tabular} \end{table}