\begin{table}%t2 \caption{\label{tab:map14}Core properties.} %\begin{center} \par \begin{tabular}{lrc ccrrc} \hline\hline\noalign{\smallskip} {Core} & {$R$} & {$\overline{\Delta V}_{13}$} &{$L_{\rm{bol}}$} & {Peak $n({\rm H}_{2})$} & {$M_{\rm LTE}$ } & {$M_{\rm vir}$ } & {$\alpha ^*$}\\ { } & {(pc)} & {($\rm{km~s}^{-1}$)} &{($10^3L_{\odot}$)} & {($10^{3}~{\rm cm}^{-3}$)} &{($M_{\odot}$)} & {($M_{\odot}$)} & {}\\ {(1)} & {(2)} & {(3)} & {(4)} & {(5)} & {(6)} & {(7)} & {(8)}\\ \hline \par 00117+6412 & 0.57 &2.58 &4.29 &5.13 & 1.8E+2 &4.8E+2 &2.7 \\ 00557+5612 & 1.08 &2.05 &1.47$^{u}$ &1.66 & 6.6E+2 &5.7E+2 &0.9 \\ 03101+5821 & $>$1.08 &2.52 &1.20 &1.76 & $>$5.8E+2 &8.6E+2 &1.5 \\ 03260+3111$^{a}$ & $>$0.23 &3.05 &0.29 &15.96 & $>$1.6E+2 &2.6E+2 &1.6 \\ 03260+3111NE$^{s}$ & 0.11 &2.51 &... &15.96 & 8.0E+1 &8.8E+1 &1.1 \\ 03414+3200 & $>$0.34 &1.92 &0.05$^{u}$ &5.35 & $>$8.5E+1 &1.6E+2 &1.8 \\ 05168+3634 & $>$2.41 &2.86 &17.13 &1.57 & $>$1.2E+4 &2.4E+3 &0.2 \\ 05168+3634SW$^{s}$ & 0.60$^{m}$ &2.61 &... &1.57 & 3.0E+3 &5.2E+2 &0.2 \\ 06067+2138 & 0.55 &3.36$^{b}$ &0.03$^{u}$ &3.83 $^{c}$ & 2.5E+2 &7.8E+2 &3.1 \\ 06103+1523 & 1.97 &2.56 &9.49 &1.02 & 2.8E+3 &1.6E+3 &0.6 \\ 07024$-$1102 & $>$0.11$^{m}$ &1.99 &0.57 &64.73$^{c}$ & $>$9.0E+0 &5.8E+1 &6.4 \\ 20067+3415 & 1.76 &3.80$^{b}$ &1.14 &1.14 & 3.9E+3 &3.2E+3 &0.8 \\ 20067+3415NE$^{s}$ & 0.45$^{m}$ &3.67 &... &1.14 & 9.7E+2 &7.5E+2 &0.8 \\ 20149+3913 & 0.43 &3.19 &0.30$^{u}$ &2.62 & 1.4E+3 &5.5E+2 &0.4 \\ 20151+3911$^{a}$ & $>$1.30 &3.83 &0.70$^{u}$ &2.62 & $>$4.1E+3 &2.4E+3 &0.6 \\ 21391+5802 & 0.32 &2.78 &0.26 &11.87$^{c}$ & 1.3E+2 &3.1E+2 &2.4 \\ 22198+6336 & 1.22 &2.21$^{b}$ &1.53$^{u}$ &2.39 & 1.7E+3 &7.5E+2 &0.4 \\ 22506+5944 & 1.31 &2.88 &6.83 &1.40 & 1.0E+3 &1.4E+3 &1.4 \\ \hline Average$^\dagger$ & 0.98 &2.80 &3.02 &4.95 & 1.9E+3 &1.1E+3 &1.3 \\ \hline \end{tabular} %\end{center} \par Note. $^{a}$~Not guide \textit{IRAS} source. Luminosity calculated based on \textit{IRAS} fluxes and distance: 03260+3111 at 0.4~kpc \citep{1998AetAS..132..211H} and 20151+3911 at 1.7~kpc \citep{2007AetA...476.1243M}. $^{b}$~Average spectrum fitted with two Gaussian profiles, list the stronger one. $^{c}$~No $^{12}$CO data, density calculated by assuming reasonable $T_{\rm ex}$ (see text). $^{m}$~Core's angular diameter comparable to beamwidth, marginally resolved. $^{s}$~Sourceless core. $^{u}$~Upper limit. $^\dagger$~Average calculating does not include values of marginally resolved cores, except for the line width column. $^*$~$\alpha = M_{\rm vir}$/$M_{\rm LTE}$. \end{table}