\begin{table}%t2 \par \caption{\label{18COtable}Physical parameters of ${\rm C^{18}O} (J=1{-}0)$ clumps.} %\centerline { \begin{tabular}{c c c c c c c c c c c c c c c} \hline \hline\\[-3.2mm] {Clump}&{$l$$^{{\rm 1}}$}&{$b$$^{{\rm 1}}$}&{$\alpha$$^{{\rm 1}}$}&{$\delta$$^{{\rm 1}}$}&{$T_{\rm a}^*$}&{$\delta v$$^{{\rm 2}}$}&{$V_{{\rm LSR}}$}&{$r$}&{$N({\rm H_2}$)}&{$n({\rm H_2}$)}&{LTE mass}&{Virial mass}&{$M_{\rm LTE} / M_{\rm vir}$}&{associated of} \\ {}&{(degree)}&{(degree)}&{(J2000.0)}&{(J2000.0)}&{(K)}&{(km s$^{-1}$)}&{(km s$^{-1}$)}&{(pc)}&{($\times 10^{22}$ cm$^{-2}$)}&{($\times 10^{4}$ cm$^{-3}$)}& ($M_{\rm LTE}$) {($M_{\odot}$)} &($M_{\rm vir}$)$^{{\rm 4}}$ {($M_{\odot}$)}&{}& {\element[][13]{CO} cloud} \\ \hline 1 &137.54 &1.28 &02 55 03 &+60 35 49 &0.92 &1.47 &--38.1 &0.21 &2.0 &1.4 &55 &110 &0.50 &cloud~1 \\ 2 &137.62 &1.36 &02 55 53 &+60 37 21 &1.11 &1.54 &--39.3 &0.85 &2.3 &0.47 &550 &380 &1.4 &cloud~4 \\ 3 &137.66 &1.53 &02 56 55 &+60 45 33 &1.02 &1.20 &--38.3 &0.35 &2.0 &1.2 &67 &85 &0.79 &cloud~4 \\ 4 &137.71 &1.48 &02 57 01 &+60 41 46 &1.32 &1.50 &--38.7 &0.61 &3.0 &1.3 &170 &180 &0.94 &cloud~4 \\ 5 &137.78 &1.46 &02 57 27 &+60 38 46 &0.91 &0.96 &--39.3 &0.33 &3.7 &0.97 &110 &68 &1.6 &cloud~4 \\ 6 &138.14 &1.69 &03 00 56 &+60 40 46 &1.38 &1.26 &--38.1 &0.46 &3.3 &1.5 &230 &130 &1.8 &cloud~6 \\ 7 &138.29 &1.55 &03 01 28 &+60 29 05 &2.60 &1.79 &--38.3 &0.84 &5.8 &1.8 &740 &370 &2.0 &cloud~7 \\ 8 &138.43 &1.60 &03 02 40 &+00 00 00 &1.50 &1.33 &--38.6 &0.39 &3.3 &1.5 &180 &140 &1.3 &cloud~7 \\ 9 &138.50 &1.65 &03 03 21 &+60 28 17 &1.94 &1.68 &--37.9 &0.39 &4.3 &2.6 &130 &160 &0.81 &cloud~7 \\ \hline \end{tabular}} \par \medskip $^{1}$ The coordinates indicate the peak position. $^{2}$ {\it FWHM} of the Gaussian fit to the observed spectra. $^{3}$ The velocity corresponding to the peak intensity of the Gaussian fit to the observed spectra. $^{4}$ $M_{\rm vir} = 210 \times r \times \delta~v$ ($M_{\odot}$). \end{table}