\begin{table}%t3
%\centering
\par
\caption{\label{SEDfit}SED fitting results.}
\par
\begin{tabular}{lcccccccccccccc}
\hline \hline \noalign{\smallskip}
O-rich stars  \\
\hline\noalign{\smallskip}
Name & $T_{\rm eff}$ & $T_{\rm c}$ & $\mathbf{\tau} _{\lambda}$ & $n$ & $D$ & $V_{\rm gas}$ & $L$ (${\times}10^{4}$) &$\dot{M}$ ($\times$$ 10^{-6}$) & $M_{\rm d}$ (${\times}10^{-5}$)& ${M}$ ($\times 10^{-3}$) & Am. Silicate & Alumina & Fe & $\dot{M}_{\rm ref}$ (${\times}10^{-6}$) \\ 
&  [K]          & [K]           &          &      & [kpc] &[km~s$^{-1}$]&$L_{\sun}$&[$M_{\sun}$/yr]& [$M_{\sun}$] & [$M_{\sun}$] & [\%]  &[\%] &[\%]	 & [$M_{\sun}/$yr]  \\
\hline
WX~Psc & 2500 & 1010 & 9 & --2.0 & 0.75$^{a}$  & 20$^{b}$ & 1.1& 13 & 17 & 36  & 98 Ossen. &  & 02 & 0.3$-$8$^{b}$  \\
 $o$~Cet & 2600  & 1000 & 0.12 & --1.9 & 0.128$^{c}$ & 8$^{b}$ &1.4& 0.11  & 0.11 & 0.11 & 100 Dorsch. &  & & 0.5$^{k}$  \\
 VY~CMa & 2500 & 1100 & 13 & --2.1 & 1.14$^{r}$ & 47$^{b}$ &27.5& 203 & 600 & (...) & 98 Ossen. &  & 02 & 100$^{n}$$-$300$^{o}$  \\
 IRAS 16342$-$3814 & 2600 & 1000 & 480 &--2.2 & 2$^{i}$ &46$^{h}$ &0.04& 319 & 128 & {\textless}140 & 75 Ossen. &  & 25 &300$^{i}$ \\
 AFGL~5379 & 2600 & 700 & 52 &--2.3 & 1.19$^{d}$ & 24$^{b}$ &0.5& 46 & 97 & {\textless}250 & 97 Dorsch. &  & 03 & 9$-$200$^{q}$\\ 
 IRC~$+$10420 (ISO) & 7000 & 750 & 5 & --2.2 &5$^{e}$ & 42$^{b}$ &47& 693 & 1980 & {\textless}4400 & 99.5 Dorsch. &  & 0.5 & 700$-$900$^{m}$  \\
 IRC~$+$10420 (LRS)     & 7000 & 750 & 4  & --2.2 & 5$^{e}$&  42$^{b}$&39 & 260 & 522 &{\textless}1600 & 90 Dorsch. & 08 & 02 & 700$-$900$^{m}$ \\
 $\pi$~Gru & 3000 & 900 & 0.04 & --2.0 &0.153$^{c}$ & 11$^{g}$ &1.04& 0.05 & 0.01 & 0.06 & 50 Ossen. & 50 &  & 0.2$-$0.7$^{l}$  \\
\hline \\[-3mm]
C-rich stars  \\\hline
%\hline
Name & $T_{\rm eff}$ & $T_{\rm c}$ & $\mathbf{\tau}_{\lambda}$ & $n$ & $D$ & $V_{\rm gas}$ & $L$ (${\times}10^{4}$)&  $\dot{M}({\times}10^{-6}$) & $M_{\rm d}$ (${\times}10^{-5}$)& ${M}$ (${\times}10^{-3}$) & Am. C & SiC & MgS & $\dot{M}_{\rm ref}$(${\times}10^{-6}$) \\ 
&  [K]  & [K]   &  &  & [kpc] &[km~s$^{-1}$]&$L_{\sun}$&[$M_{\sun}$]&[$M_{\sun}$] & [$M_{\sun}$] & [\%]   &[\%] &[\%] & [$M_{\sun}$/yr] \\
\hline
CW~Leo & 2650 & 1050 & 25 & --2.3 &0.135$^{j}$ & 17$^{f}$ &0.9& 7 & 1.2 & 6.2 & 66 & 12 & 22 & 22$^{j}$ \\
AFGL~3068 & 2650  & 1000  & 135 & --2.5 &1.05$^{d}$ & 16$^{f}$ &1.4& 110 & 3.6 & \textless\ 300 & 78 & 04 & 18 & 20$-$62$^{p}$ \\
\hline 
\end{tabular}
\tablebib{{a}{van Langevelde et~al. (\cite{van1990});} {b}{Kemper et~al. (\cite{Kemper2003});} {c}{Hipparcos (Perryman \& ESA \cite{Perryman1997})}; {d}{Yuasa et~al. (\cite{Yuasa1999})}; {e}{Jones et~al. (\cite{Jones1993})}; {f}{Groenewegen et~al. (\cite{Groenewegen1996})}; {g}{Knapp et~al. (\cite{Knapp1999});} {h}{He et~al. (\cite{He2008})}; {i}{Sahai et~al. (\cite{Sahai1999});} {j}{Groenewegen et~al. (\cite{Groenewegen1998b});} {k}{Loup et~al. (\cite{Loup1993});} {l}{Groenewegen \& de~Jong (\cite{Groenewegen1998a});} {m}{Dinh-V-Trung et~al. (\cite{Dinh2009});} {n}{Jura \& Kleinmann (\cite{Jura1990});} {o}{Harwit et~al. (\cite{Harwit2001});} {p}{Ramstedt et~al. (\cite{Ramstedt2008});} {q}{Kastner (\cite{Kastner1992});} {r}{Choi et~al. (\cite{Choi2008}).}  }
\tablefoot{$T_{\rm eff}$ is the effective temperature, $T_{\rm c}$ the dust condensation temperature, $\mathbf{\tau} _{\lambda}$ is the optical depth at 0.55~$\mu$m, n is the density power index, $D$ the distance to the star,  $V_{\rm gas}$ the terminal velocity derived from CO line measurements, $L$ the luminosity, $\dot{M}$ the mass loss rate, $M_{\rm d}$ is the dust mass , ${M}$ the total dust and gas mass loss, $\dot{M}_{\rm ref}$ the mass loss derived from previous studies.}
\vspace*{1cm}
\end{table}