\begin{table}%t1
\caption{\label{tab:modelsets}Physical parameters corresponding to the most important of our binary population models. (A~full list of all our model sets can be found in Table~\ref{tab:The-full-list-of-population-parameters}.)}
%\centering
 \small
\begin{tabular}{cc}
\hline\hline 
Model set & Physical parameters \\
 & (differences from model set \protect $A$)\\
\hline
$A$ & --\\
{\it Ap5}, {\it Ap7} & $\left[{\rm C}/{\rm Fe}\right]_{{\rm min}}=0.5$ and $0.7$
respectively\\
{\it A1}, {\it A2} & $\xi_{13}=0.1$ and $0.01$ respectively\\
{\it B} & Bondi-Hoyle efficiency $\alpha_{{\rm BH}}=5$\\
{\it C} & common envelope accretion $0.05~M_{\odot}$\\
{\it D} & no thermohaline mixing\\
{\it E} & $\Delta M_{{\rm c,min}}=-0.07~M_{\odot}$, $\lambda_{{\rm min}}=0.8$\\
{\it F} & $M_{{\rm env},{\rm min}}=0~M_{\odot}$\\
{\it G} & 
$\Delta M_{{\rm c,min}}=-0.1~M_{\odot}$, $\lambda_{{\rm min}}=0.8$,\\
 & $M_{{\rm env},{\rm min}}=0~M_{\odot}$, $\xi_{{\rm 13}}=0.1$
\\
{\it H} & as model $G$, with: \\
& common envelope accretion $0.05~M_{\odot}$ \\
& no thermohaline mixing \\
\hline
\end{tabular}
\end{table}