\begin{table}%t3
%\centering
\par
\caption{\label{tabsio}Turbulence support, SiO outflow, and gravitational infall of the most massive dense cores of NGC~6334 - NGC~6357.}
\par
\begin{tabular}{c c c c c c c c c c c c l}
\hline \hline \noalign{\smallskip}
Core   &$M_{\rm vir}$& $f_{\rm turb}$ & $V_{\rm lsr}$& $T_{\rm SiO}$ & $FWHM_{\rm SiO}$ & $\Delta v_{\rm outflow}$ & $\int T _{\rm sio}{\rm d}v$ & $\delta V$ & $\delta~V$ & $T_{\rm B}$/$T_{\rm R}$& $T_{\rm B}$/$T_{\rm R}$ & Possible \\ 
number             &      &    &  &   &   &   &  & HCO$^{+}$  & HNC & HCO$^{+}$ & HNC & nature \\
& (\msun) &  &(km~s$^{-1}$)  & (K)  & (km~s$^{-1}$) & (km~s$^{-1}$)  & (K~km~s$^{-1}$) &  &  &  & & \\
\hline 
\bf{3} &  120    & 2.51&  $-$10.77&   0.23 &    2.8  &    7.00 & $  0.35 \pm  0.08  $  &  $-$5.01& $-$5.23&    -- &        --   &C\hii\  region \\
9 &  160    & 2.46&  $-$9.46 &   0.42 &    5.8  &    23.2 & $   2.3  \pm 0.09  $  &  $-$5.52& $-$5.23&    -- &   4.17       &IR-Quiet protostar \\
18 &  328    & 3.60&  $-$4.19 &  --    &    --   &    --   & --                    &  $-$0.54& $-$0.39&     3.87  &   2.64          &IR-Quiet protostar \\
23 &  139    & 2.07&  $-$5.36 &  --    &    --   &    --   &  --                   &  $-$0.27& $-$0.53&    -- &   --        &starless core  \\ 
\bf{28} &  168    & 3.02&  $-$6.03 &  --    &    --   &    --   & --                    &  $ $1.48& $ $1.48&    -- &   0.90          &starless core  \\
\bf{29} &  461    & 5.24&  $-$5.94 &   0.30 &    6.2  &    17.8 & $   1.4  \pm 0.09  $  &  $ $0.17& $ $0.21&    -- &   --        &IR-Bright protostar \\
   32 &  166    & 2.20&  $-$2.36 &  --    &    --   &    --   & --                    &  $ $0.32& $ $0.16&     0.16  &   --        &starless core  \\
   35 &  142    & 2.67&  $-$4.77 &   0.29 &    5.4  &    10.3 & $  0.8   \pm  0.09 $  &  $ $0.20& $ $0.07&    -- &   --        &IR-Quiet protostar \\
\bf{37} &  424    & 4.08&  $-$5.09 &   0.29 &    6.6  &    11.8 & $   1.2  \pm 0.09  $  &  $-$0.03& $ $0.05&    -- &   --        &IR-Quiet protostar \\
\bf{38} &  195    & 3.08&  $-$2.48 &   0.44 &    4.9  &    13.9 & $   1.8  \pm 0.10  $  &  $ $0.61& $ $0.96&    -- &   --        &C\hii\  region \\
\bf{43} &  216    & 3.62&  $+$0.07 &   0.30 &    3.9  &    9.1  & $  0.99 \pm  0.09  $  & $-$1.03*& $-$0.93&    -- &   --        &IR-Quiet protostar \\
   44 &  164    & 2.55&  $-$2.11 &   0.16 &    3.3  &    6.0  & $  0.55 \pm  0.09  $  &  $-$0.23& $-$0.23&    -- &   --        &IR-Quiet protostar \\
   46 &  168    & 2.97&  $-$5.11 &  --    &    --   &    --   & --                    &  $-$0.02& $ $0.04&    -- &  10.17          &starless core  \\
\bf{47} &  215    & 2.82&  $-$0.83 &   0.13 &     0.3 &    9.9  & $  0.57  \pm  0.08$   &  $ $0.11& $ $0.04&    -- &   --        &C\hii\ region \\
\bf{51} &  1446   & 6.07&  $-$3.54 &   0.15 &    5.7  &    11.3 & $  0.82 \pm  0.09  $  &  $ $0.30& $-$0.83&     0.89  &   1.08          &C\hii\  region \\
   52 &  691    & 7.39&  $-$2.35 &   0.10 &    5.9  &    8.4  & $  0.59  \pm 0.07  $  &  $-$0.10& $-$0.21&    -- &   0.17          &IR-Quiet  protostar \\
   54 &  85     & 2.76&  $-$4.15 &   0.13 &    10.7 &    17.3 & $   1.3 \pm  0.08  $  & $-$2.13*& $-$2.06&    -- &   --        &IR-Quiet protostar \\
   56 &  205    & 2.88&  $-$3.40 &  --    &    --   &    --   & --                    &  $ $0.34& $ $0.65&     0.37  &   0.88          &starless core  \\
   58 &  391    & 4.22&  $-$4.35 &  --    &    --   &    --   & --                    & $ $0.18*& $ $0.05&     0.44  &   0.29          &starless core  \\
   60 &  332    & 5.36&  $-$3.98 &   1.08 &    5.8  &    23.2 & $   7.0 \pm  0.29  $  &  $-$0.62& $-$0.52&     1.70  &   1.56          &IR-Quiet protostar \\
   61 &  326    & 3.93&  $-$2.97 &   0.78 &    4.5  &    29.0 & $   4.8 \pm  0.15  $  &  $ $0.44& $ $0.39&     0.40  &   0.46          &IR-Quiet protostar \\
\bf{62} &  525    & 7.29&  $-$7.06 &   0.57 &    6.0  &    24.1 & $  3.8 \pm    0.14 $  &  $-$0.21& $-$0.18&     6.10  &   9.93          &UC\hii\  region \\
\bf{63} &  997    & 7.54&  $-$4.77 &   2.41 &    6.6  &    66.3 & $  25.4 \pm  0.40  $  &  $-$0.35& $-$0.13&     2.94  &   --        &IR-Quiet protostar \\
   66 &  300    & 3.41&  $-$6.29 &  --    &    --   &    --   & --                    & $ $0.01*& $ $0.01&     0.69  &   0.60          & starless core  \\
   78 &  216    & 3.04&  $-$4.11 &  --    &    --   &    --   & --                    & $-$0.20*& $-$0.20&     3.50  &   3.98          & starless core  \\
   81 &  234    & 3.12&  $+$1.93 &  --    &    --   &    --   & --                    &  $ $0.29& $ $0.29&    -- &   --        & starless core  \\
\bf{85} &  295    & 4.47&  $-$2.50 &   0.16 &    --   &    13.1 & $  0.84    \pm 0.07$  &  $-$0.59& $-$0.06&     8.87  &   --        &HC\hii\  region?\\
   98 &  328    & 4.06&  $-$4.14 &  --    &    --   &    --   &--                     &  $-$0.19& $-$0.06&    -- &   --        &IR-Quiet protostar \\
\bf{109} &  253    & 2.66&  $-$3.35 &  --    &    --   &    --   & --                    &  $ $0.09& $ $0.02&     0.34  &   0.25          &C\hii\  region \\
\bf{110} &  130    & 2.26&  $-$5.90 &  --    &    --   &    --   &--                     &  $-$0.24& $-$0.16&    -- &   --        &C\hii\  region \\
  112 &  194    & 3.31&  $-$8.48 &  0.007 &    4.2  &    6.2  & $  0.30 \pm  0.06  $  &  $-$0.07& $ $0.09&    -- &   --        &IR-Quiet protostar \\
  115 &  92     & 2.28&  $-$5.47 &  --    &    --   &    --   &--                     &  $-$0.17& $-$0.09&     1.06  &   0.75          &starless core  \\
\bf{118} &  313    & 3.05&  $-$3.28 &  0.10  &    --   &    3.6  & $  0.17  \pm 0.08  $  & $-$0.04*& $-$0.04&     2.12  &   1.24          &IR-Quiet protostar \\
\bf{122} &  286    & 3.53&  $-$3.88 &  0.067 &    --   &    4.7  & $  0.38 \pm  0.07  $  &  $-$0.10& $ $0.05&     0.09  &   --        &IR-Quiet protostar \\
\bf{130} &  --     &--   &  $-$7.52 &  --    &    --   &    --   &--                     &  $ $ -- & $ $ -- &     0.31  &   0.36          &C\hii\  region \\ 
  132 &  155    & 2.88&  $-$3.18 &  --    &    --   &    --   & --                    &  $-$0.01& $-$0.07&    -- &   --        &starless core  \\
  137 &  --     &--   &  $-$6.87 &  --    &    --   &    --   & --                    &  $ $ --*& $ $ -- &     1.05  &   0.77          &starless core  \\
  141 &  359    & 3.43&  $-$2.76 &  --    &    --   &    --   & --                    &  $-$0.28& $-$0.18&    -- &   1.81          &IR-Quiet protostar \\
  149 &  193    & 2.81&  $-$3.43 &  --    &    --   &    --   & --                    &  $ $0.17& $ $0.24&     0.13  &   --        &starless core  \\
  150 &  136    & 3.32&  $-$4.68 & 0.0086 &   0.97  &    2.2  & $  0.10 \pm  0.06  $  &  $-$0.30& $-$0.14&    -- &   --        &IR-Quiet protostar \\
  158 &  438    & 3.70&  $-$1.74 &  --    &    --   &    --   & --                    & $-$0.35*& $-$0.15&     2.18  &   2.49          &starless core  \\
  161 &  276    & 3.75&  $-$1.98 &  --    &    --   &    --   & --                    &  $-$0.09& $ $0.00&     4.93  &        --   &starless core  \\          
\hline
\end{tabular}
\tablefoot{Column~1: the core number as in Table~\ref{tab_a1} (numbers in boldface indicate the $M > 200$~\msun~cores). Column 2: the virial mass (see Sect.~4.2.2). Column 3: the internal turbulence (see Sect.~4.2.1). Column~4: the systemic velocity deduced from $^{13}$CS and/or H$^{13}$CO$^{+}$. Columns~5 to 8: the peak line intensity, the line width at half maximum, full line width at the base and integrated intensity of the SiO emission. Columns~9 to 12 (see Sect.~4.2.4): the asymetric parameter and the blue to red peak ratio of the HCO$^{+}$ and HNC lines. 
Asterisk in the $\delta$V$_{HCO^{+}}$ column indicates dense cores suspected to have several components present along the line of sight. Column~13: the possible nature of the source: Compact \hii\  region (C\hii\  region), ultra-compact \hii\  region (UC\hii\  region), hyper-compact \hii\  region (HC\hii\  region), IR-quiet protostar, IR-bright protostar, or starless core.}
\vspace*{3mm}
\end{table}