\begin{table}%t1 \caption{\label{n2h+}Parameters of N$_2$H$^+$(1--0) emission peaks.} %\centerline {\small \begin{tabular}{lrrrrrrrr} \hline \hline \# & Offset$^a$ & $T_{\rm{peak}}$ & $v$ & $\Delta v$ & $\tau$ & $N_{\rm{N_2H^+}}$ & $M_{\rm{vir}}^b$ & av.~$\rho$ \\ & $''$ & K & km~s$^{-1}$ & km~s$^{-1}$ & & $\times 10^{13}$cm$^{-2}$ & $M_{\odot}$ & $10^5$cm$^{-3}$ \\ \hline 1 & 6.2/8.6 & 2.1 & 7.7 & 1.8 & 11.9 & $6.6\pm 0.3$ & 7.5--11.4 & 19\\ 2 & 12.1/17.8 & 0.7 & 6.9 & 0.8 & 12.7 & $1.9\pm 0.3$ & 0.6--0.9 & 12\\ $3_1$& 0.7/4.3 & 1.5 & 7.3 & 0.5 & 7.0 & $0.9\pm 0.1$ & 0.3--0.4 & 5.9\\ $3_2$& 0.7/4.3 & 0.4 & 8.3 & 0.8 & 16.3 & $2.1\pm 0.5$ & 0.6--0.9 & 14\\ 4 & --10.1/--9.0 & 2.3 & 8.1 & 1.1 & 6.5 & $2.3\pm 0.2$ & 1.3--1.9 & 15\\ 4a & --9.9/--5.8 & 2.3 & 7.7 & 0.7 & 7.8 & $1.7\pm 0.1$ & 0.5--0.7 & 11\\ 5 & --8.6/--4.5 & 2.2 & 7.7 & 0.8 & 7.1 & $1.9\pm 0.1$ & 0.7--1.1 & 12\\ 6 & --5.7/0.7 & 1.3 & 8.2 & 0.7 & 12.6 & $2.0\pm 0.1$ & 0.5--0.7 & 13\\ 7 & --3.6/5.3 & 1.3 & 8.1 & 0.6 & 5.1 & $0.7\pm 0.1$ & 0.3--0.5 & 4.6\\ 8 & --2.9/8.2 & 4.3 & 8.0 & 0.7 & 0.1 & $0.8\pm 0.1$ & 0.5--0.7 & 5.2\\ 9 & --1.0/13.0 & 0.9 & 8.2 & 0.5 & 8.3 & $0.9\pm 0.2$ & 0.3--0.4 & 5.9 \\ 10 & --0.1/17.8 & 2.2 & 8.1 & 0.5 & 2.0 & $0.4\pm 0.1$ & 0.3--0.5 & 2.6 \\ $11_1$ & 4.6/23.7& 1.4 & 7.6 & 0.5 & 1.1 & $0.3\pm 0.1$ & 0.3--0.5 & 2.0 \\ $11_2$ & 4.6/23.7& 0.6 & 8.6 & 0.8 & 4.9 & $0.7\pm 0.1$ & 0.6--0.9 & 4.6\\ 12 & --14.2/--11.1 & 2.0 & 7.7 & 1.2 & 5.7 & $2.0\pm 0.2$ & 1.5--2.2 & 13 \\ 13 & --5.4/--7.4 & 1.5 & 7.8 & 0.7 & 10.4 & $1.8\pm 0.1$ & 0.5--0.7 & 12\\ 14$_1$& --0.6/--5.2 & 0.5 & 7.8 & 1.0 & 10.7 & $1.9\pm 0.2$ & 1.0--1.5 & 12\\ 14$_2$& --0.6/--5.2 & 2.6 & 8.8 & 0.7 & 0.1 & $0.3\pm 0.1$ & 0.5--0.7 & 2.0\\ 15 & --17.6/--4.9 & 2.6 & 8.9 & 0.5 & 0.9 & $0.3\pm 0.3$ & 0.3--0.4 & 2.0\\ 16 & --24.5/3.3 & 2.8 & 6.8 & 1.0 & 3.7 & $1.4\pm 0.1$ & 0.9--1.4 & 9.2\\ 17 & --20.7/5.7 & 3.1 & 6.8 & 1.0 & 0.1 & $0.6\pm 0.2$ & 1.0--1.6 & 3.9\\ \hline \end{tabular}} \par \medskip The subscripts associated with sources 3, 11 and 14 correspond to two different velocity components required for the spectral fits.\\ $^a$ The offsets are given with respect to the phase center RA[J2000] 19$^{\rm h}$19$^{\rm m}$50.169$^{\rm s}$ and Dec[J2000] 14$^{\circ}$01$'$13.75$''$.\\ $^b$ The virial masses were calculated following \citet{maclaren1988} for $1/r$ and $1/r^2$ density distributions, resulting in the ranges of values. All source radii were approximated with half of the average N$_2$H$^+$ synthesized beam of $\sim $$3.1''$. Only for peak one we used a source radius of $3.5''$. \end{table}