\begin{table}%t1
\caption{\label{General}Source list, JCMT and SEST observations; general information.}
%\centering
\par
\begin{tabular}{l cc l l c  c c l }
\hline\hline\noalign{\smallskip}
& RA (J2000) 	& Dec (J2000) 			& $V_{\rm LSR}$ 		&        		& Distance 	& Dist. source 	 & Dist. HH &Proposed  \\
 Object   	&  (h m s) 	& ($^{\rm o}$ $'$ $''$) 	& (km~s$^{-1}$)	&  Location 	& (pc) 		& to HH (pc)\tablefootmark{a,b}  	& 
to HCO$^+$ (pc)\tablefootmark{b,c}  
 & exciting source \\
\hline
HH~267 &03 24 03.0 	&$+$31 00 29 	& 4.5 	& L1448	  	& 300 	&2.53 	&--			&L1448C\\
HH~268 &03 24 22.1 	&$+$30 48 11 	& 4.5 	& L1448	  	& 300 	&1.35 	&--			&L1448~IRS1\\
HH~337A&03 28 26.3 	&$+$31 25 53 	& 4.0 	& NGC~1333  	& 300 	&0.99	&0.03		&333 star\\
HH~278 &03 26 59.4 	&$+$30 25 58 	& 7.0 	& L1455/L1448 & 300 	&2.47 	&--			&L1448NB  \\
HH~366 &03 48 29.8	&$+$32 55 36 	& 5.0 	& Barnard 5 	& 300 	&1.28 	&0.01 		&B5 IRS 1 \\
HH~427 &03 30 37.7 	&$+$30 21 56 	& 6.0 	& Barnard 1 	& 300  	&N/A 		&N/A		&Not known \\
HH~211 &03 43 56.8 	&$+$32 00 50 	& 9.2 	& IC~348    	& 300 	&0.08 	&0.01 		&HH 211-mm \\
HH~462 &03 54 05.0 	&$+$38 10 35	&$-3.5$	& Perseus 	& 300 	&0.01	&0.04		&IRAS~03507+3801 \\
HH~362A&04 04 24.1 	&$+$20 20 41 	& 7.2 	& L1489	   	& 140 	&0.20	&--			&IRAS~04106+2610 \\
HH~464 &04 10 42.4 	&$+$38 07 39	&$-3.5$	& L1473	   	& 350 	&0.07	&0.05			&PP~13N \\
HH~276 &04 22 07.3 	&$+$26 57 26 	& 6.5 	&Taurus-Auriga& 140	&1.80	&--			&IRAS~04189+2650  \\
HH~29  &04 31 27.6 	&$+$18 06 24 	& 6.6 	& L1551	  	& 140 	&0.11	&0.01		&L1551~IRS 5       \\
HH~240 &05 19 40.7 	&$-$05 51 44 	& 8.5 	& L1634	  	& 460 	&0.28 	&0.11		&IRAS 05173$-$0555 \\
HH~43  &05 38 10.4 	&$-$07 09 25 	& 8.5 	& L1641	  	& 460 	&0.57 	&0.17		&IRAS~05355$-$0709C\\
HH~38  &05 38 21.8 	&$-$07 11 38 	& 8.5 	& L1641	  	& 460 	&1.06  	&0.07		&IRAS~05355$-$0709C\\
HH~272 &06 12 48.4	 	&$-$06 11 21 	&11.0	& L1646	  	& 830 	&0.46 	&0.08		&IRAS~06103$-$0612 \\
HH~47C &08 25 33.0 	&$-$51 01 37 	& 6.0 	& Gum Nebula	& 450 	&0.26 		&--			& HH~46/47~IRS      \\
HH~75  &09 11 38.5 	&$-$45 42 28	&$-0.9$	& Gum Nebula	& 450 	&-- 		&--			&IRAS~09094$-$4522 \\
HH~49  &11 06 00.1 	&$-$77 33 36 	& 5.3 	& Cha I	  	& 160 	&2.69 		&--	 		&Cha-MMS1         \\
HH~52-53&12 55 06.4	&$-$76 57 46 	& 4.0 	& Cha II    	& 165 	&1.39	&--			&IRAS~12496$-$7650 \\
HH~54  &12 55 49.5 	&$-$76 56 08 	& 4.0 	& Cha II    	& 165 	&1.90	&--			&IRAS~12496$-$7650\\
HH~77  &15 00 49.0 	&$-$63 07 46	&$-5.0$	& Circinus  	& 700 	&0.63 	&0.06		&IRAS~14564$-$6254 \\
\par
\hline
\end{tabular}
\par
\tablefoot {\tablefoottext{a}{Column (7) lists the distance between the exciting source and the HH Object.}      
\tablefoottext{b}{``N/A'' indicates that the exciting source is not known and no values can be deduced, whereas a ``--'' indicates that no HCO$^+$ emission was seen.}
\tablefoottext{c}{Column (8) lists the distance between the proposed HH Object and the peak emission of HCO$^+$ (3--2) seen.} }
\vspace*{-2mm}{\tablebib{HH29: \citet{Moriarty06}; HH38--43: \citet{Stanke00}; 
HH49: \citet{Reipurth96}; HH52--53 and HH54: \citet{Knee92}; 
HH47: \citet{Sahu89}; HH75 and HH77: \citet{Cohen90}; 
HH211: \citet{McCaughrean94}; HH240: \citet{Davis97};
HH267: \citet{Bally97};  HH268: \citet{Eisloffel00}; HH272: \citet{Carballo92};
HH276: \citet{Wu02}; HH278: \citet{Eisloffel00}; HH337A: \citet{Bally96b};
HH362: \citet{Alten97}; HH366: \citet{Bally96a}; HH427: \citet{Yan98}; 
HH462 and HH464: \citet{Aspin00}.}} 
\end{table}