\begin{table}%t3
\caption{\label{modeltable}Parameters of the simulations, all with solar metallicity.}              
\par
%\centering
\par
\begin{tabular}{c c c c c c c c}        
\hline\hline \noalign{\smallskip}                 
 Model & Stellar  & $M$         & $L$      &$R$          & $T_{\rm{eff}}$ & log$g$   \\
name   & type            & $[M_\odot]$ &$[L_\odot]$  & $[R_\odot]$   & [K]        & [cgs] \\
\hline
M18\tablefootmark{a}    & Mira     & 1.2  & 4840 & 210 & 3310 & -- \\
st28gm06n06\tablefootmark{b} & AGB & 1  & 6935& 429 & 2542 & --0.83 \\
st35gm03n07\tablefootmark{c} & RSG & 12 & 93~000& 832 & 3490 & --0.34 \\
\hline                         
\end{tabular}
\tablefoot {\tablefoottext{a}{1D model; the radius is the Rosseland radius $R=0.81~R_{\rm p}$ at Mira phase $\approx$0.75; \citep{2004MNRAS.355..444I};}
\tablefoottext{b}{3D model; \cite{2008AetA...483..571F};}
\tablefoottext{c}{3D model; \cite{2009AetA...506.1351C}.}}
\end{table}