\begin{table}%t2
\par
%\centering
\par
\caption{Comparison of observed SWB parameters to those calculated from a simple
time-evolution model of a SWB formed by the wind of a single~O5.5V
star, chosen to match the observed wind luminosity~$L_{\rm w}$ at the
minimum age of the bubble ($t=1.4$~Myr). Model is from \citet{mck84}.
The stall
velocity and age for the bubble are near the lower and upper limits
of those same parameters as measured, respectively. The stall radius
is~30\% larger than the observed radius, but is within uncertainties.
The~SWB surrounding 3C~434.1 is apparently in its early stages of dissipation.
\label{param2}}
\begin{tabular}{ccc}
\hline\hline
Parameter&
Model&
Observed\\
\hline
$L_{\rm w}$(10$^{36}$~erg s$^{-1}$)&
3.5&
5.1\\
$L_{\rm w}^{*}$&
2.73 (at $t=0$)&
3.26 (at $t=1.4$ Myr)\\
$S_{49}$(10$^{49}$ photons s$^{-1}$)&
2.3&
3.0\\
Stall Radius $R_{\rm b}$ (pc)&
5$0\pm 10$&
3$4\pm 7$\\
$v_{\rm e}$ at stall (km s$^{-1}$)&
$11.4 \pm 2.3$&
14\\
$t_{\rm stall}$ (10$^{6}$~yr)&
$2.6\pm 0.5$&
1.4--2.6\\
\hline
\end{tabular}
\end{table}