\begin{table}%t1
%%\centering

\par
\caption{\label{tb:pargrid}Crystalline silicate fractions for a range of model parameters.}
\begin{tabular}{cccccccccccccccc}
\hline\hline \noalign{\smallskip}
& \multicolumn{15}{c}{\rule{0pt}{1em}$\Omega_0=10^{-14}$ \ps, $\cs=0.19$~km~\ps} \\
\hline
\rule{0pt}{1em}$t$ & \multicolumn{15}{c}{$R$ (AU)} \\
%\cline{2-16}
\rule{0pt}{1em}(Myr) & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 \\
\hline
& \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.20$, $M_\el{d}=0.012$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.50$, $M_\el{d}=0.074$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=1.0$, $M_\el{d}=0.26$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=5.0$, $M_\el{d}=2.3$}\\
\hline
1.0 & 19.7 & 20.1 & 21.5 & & 6.7 & 6.0 & 5.5 & & 7.6 & 3.8 & 1.9 & & 17.0 & 2.9 & 0.4 \\
1.6 & 21.1 & 21.3 & 22.2 & & 6.1 & 5.8 & 5.7 & & 5.3 & 3.4 & 2.3 & & 23.0 & 3.9 & 0.4 \\
3.1 & 22.9 & 23.0 & 23.4 & & 5.9 & 5.8 & 5.9 & & 3.3 & 2.6 & 2.2 & & 24.6 & 4.4 & 0.6 \\
\hline\hline
& \multicolumn{15}{c}{\rule{0pt}{1em}$\Omega_0=10^{-14}$ \ps, $\cs=0.26$~km \ps} \\
\hline
\rule{0pt}{1em}$t$ & \multicolumn{15}{c}{$R$ (AU)} \\
%\cline{2-16}
\rule{0pt}{1em}(Myr) & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 \\
\hline
& \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.20$, $M_\el{d}=0$~\tablefootmark{a}} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.50$, $M_\el{d}=0.037$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=1.0$, $M_\el{d}=0.13$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=5.0$, $M_\el{d}=1.9$}\\
\hline
1.0 & \ldots & \ldots & \ldots & & 32.1 & 32.3 & 33.8 & & 17.4 & 16.0 & 15.1 & & 54.1 & 9.3 & 1.2 \\
1.6 & \ldots & \ldots & \ldots & & 33.3 & 33.5 & 34.4 & & 16.4 & 15.7 & 15.4 & & 37.5 & 9.7 & 2.2 \\
3.1 & \ldots & \ldots & \ldots & & 35.1 & 35.3 & 35.7 & & 16.0 & 15.8 & 15.8 & & 16.5 & 6.1 & 3.3 \\
\hline\hline
& \multicolumn{15}{c}{\rule{0pt}{1em}$\Omega_0=10^{-13}$ \ps, $\cs=0.19$~km~\ps} \\
\hline
\rule{0pt}{1em}$t$ & \multicolumn{15}{c}{$R$ (AU)} \\
%\cline{2-16}
\rule{0pt}{1em}(Myr) & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 \\
\hline
& \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.20$, $M_\el{d}=0.051$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.50$, $M_\el{d}=0.23$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=1.0$, $M_\el{d}=0.58$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=5.0$, $M_\el{d}=4.1$}\\
\hline
1.0 & 2.1 & 1.9 & 1.6 & & 2.6 & 1.3 & 0.6 & & 4.4 & 1.3 & 0.3 & & 5.4 & 1.1 & 0.2 \\
1.6 & 1.8 & 1.7 & 1.6 & & 1.7 & 1.0 & 0.5 & & 2.9 & 1.1 & 0.4 & & 5.1 & 1.2 & 0.2 \\
3.1 & 1.6 & 1.5 & 1.5 & & 1.0 & 0.6 & 0.4 & & 1.5 & 0.6 & 0.3 & & 8.5 & 0.5 & \phantom{0}0.02 \\
\hline\hline
& \multicolumn{15}{c}{\rule{0pt}{1em}$\Omega_0=10^{-13}$ \ps, $\cs=0.26$~km \ps} \\
\hline
\rule{0pt}{1em}$t$ & \multicolumn{15}{c}{$R$ (AU)} \\
%\cline{2-16}
\rule{0pt}{1em}(Myr) & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 & & 10 & 30 & 100 \\
\hline
& \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.20$, $M_\el{d}=0.019$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=0.50$, $M_\el{d}=0.13$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=1.0$, $M_\el{d}=0.43$} & & \multicolumn{3}{c}{\rule{0pt}{1em}$M_0=5.0$, $M_\el{d}=3.5$}\\
\hline
1.0 & 12.1 & 12.0 & 12.0 & & 5.3 & 4.4 & 3.6 & & 6.2 & 3.3 & 1.7 & & 19.3 & 3.9 & 0.6 \\
1.6 & 12.0 & 12.0 & 12.0 & & 4.5 & 4.0 & 3.6 & & 4.5 & 2.6 & 1.6 & & 14.6 & 3.3 & 0.7 \\
3.1 & 12.1 & 12.1 & 12.2 & & 3.7 & 3.5 & 3.3 & & 2.7 & 1.7 & 1.3 & & \phantom{0}8.6 & 2.4 & 0.8 \\
\hline
\end{tabular}
\tablefoot{The fractions are given in per cent of the total silicate dust abundance at the indicated distance from the star ($R$) and time after the onset of collapse ($t$). The initial cloud core mass ($M_0$, in~$M_\odot$) and the disk mass at the end of the accretion phase ($M_\el{d}$, in~$M_\odot$) are listed for each combination of parameters. 
\tablefoottext{a}{No disk is formed at all for this combination of parameters.}
}
\end{table}