
\documentstyle{aa}
%\onecolumn
\newcommand{\HI}{\mbox{\,{\sc i }}} 
\begin{document}
% nearby dwarf galaxy candidates frm Karachentseva & Karachentsev 1997 
% version:  16.03.1999 , 30.7.99   
\setcounter{table}{1}  
\tiny  
%\scriptsize   
\begin{table*}
\caption{List of new Local Void dwarf candidates : HI data}
\begin{tabular}{|rccllclccl|} \hline
\multicolumn{1}{|r}{KKR}&  
\multicolumn{1}{c}{\HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{velocity}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{distance}&
\multicolumn{1}{c}{M$_{Bt}$}& 
\multicolumn{1}{c}{\HI mass}&   
%\multicolumn{1}{c}{total mass}& 
\multicolumn{1}{c}{M$_{\HI}$/L$_{B}$}& 
\multicolumn{1}{c|}{Comments}
\\ \hline   
\multicolumn{1}{|c}{No. }&
\multicolumn{1}{c}{Jy$\,$km$\,$s$^{-1}$}&
\multicolumn{1}{c}{mJy }&
\multicolumn{1}{c}{km$\,$s$^{-1}$}&
\multicolumn{1}{c}{km$\,$s$^{-1}$}&
\multicolumn{1}{c}{Mpc }&
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{10$^{7}$M$_{\odot}$}&
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c|}{  }  
 \\ \hline 
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c}{10} 
%\multicolumn{1}{c|}{11}
 \\ \hline  
&&&&&& & & & \\
 1  & & $\pm$6 & & & & & & &  \\ 
 2  & 1.26& 19$\pm$6.3& 3260$\pm$3& 57 95 96& 43.2& -17.14& 55& 0.5&   \\ 
 3 & 2.1& 110$\pm$9.6& 63$\pm$2&  18 27 28&  1.9& -9.57& 0.17& 1.58& \\
 4  & & $\pm$6.8& & & & & & &   \\  
 5  & 8.74& 74$\pm$4.2& 1470$\pm$3& 93 106 109& 19.2& -15.17& 76& 4.2& \\ 
&&&&& &&&& \\  
6  & 2.76& 61$\pm$6.8& 1546$\pm$2& 34 73 74& 19.9& -15.18& 26& 1.4& \\ 
 7  & & $\pm$6.5&  & & & & & &  \\ 
 8  & & $\pm$5.8& & & & & & &  \\ 
 9  & & $\pm$9& & & & & & &   \\ 
10 & & $\pm$10& & & & & & &  \\ 
&&&&& &&&& \\   
 11 & 2.64& 75$\pm$9& 590$\pm$3& 29 46 49 & 10.2& -13.41& 6.5& 1.8&  \\ 
 12 & 4.10& 102$\pm$8& 1793$\pm$3& 42 60 65& 24.4& -15.67& 58& 2.0& \\ 
 13 & 4.83& 49$\pm$7.9& 802$\pm$2& 39 44 47& 12.2& -14.23& 17& 2.2& \\ 
 14 & & $\pm$11& & & & & & &  \\  
15 & 1.44& 40$\pm$8.4& 1588$\pm$4& 23 44 61& 21.1& -14.47& 15& 1.6& \\ 
&&&&& &&&& \\  
16 & 2.67& 37$\pm$7.8& 1616$\pm$3& 99 109 111& 21.3& -15.72& 29& 0.95& \\  
 17 & & $\pm$8.1& & & & & & &  \\ 
 18 & 1.25& 44$\pm$7& 722$\pm$2& 38 44 45& 10.5& -14.40& 3.3& 0.36&  \\ 
 19 & & $\pm$9 & & & & & & &  \\  
20 & 4.32& 46$\pm$8& 1775$\pm$2& 80 106 108& 24.1& -15.81& 59& 1.8& \\ 
&&&&& &&&& \\  
21 & 6.12& 57$\pm$5.7& 1719$\pm$2& 82 93 94& 24.3& -15.52& 85& 3.4& \\  
 22 & 2.72& 151$\pm$10& 3261$\pm$1& 19 25 27& 44.7& -17.02& 130& 1.3& \\ 
 23 & 5.83& 66$\pm$6.5& 1084$\pm$2& 103 114 116& 16.0& -15.50& 35& 1.4& \\ 
 24 & & $\pm$12& & & & & & &  \\  
25 & 2.20& 101$\pm$10& -135$\pm$2& 14 30 35& & & & & local \HI \\ 
&&&&& &&&& \\  
26 & 2.31& 59$\pm$7& 2251$\pm$2& 60 71 72& 31.6& -15.66& 54& 1.9& \\ 
 27 & & $\pm$6.7& & & & & & & \\ 
 {\it28} & & $\pm$8.1& & & & & & & \\ 
 {\it29} & & $\pm$8.4& & & & & & & \\ 
{\bf30} & 4.90& 68$\pm$5.8& 1484$\pm$2& 80 87 91 & 21.4& -15.35& 53& 2.5& \\ 
&&&&& &&&& \\  
{\it31} & & $\pm$11& & & & & & & \\ 
 {\it32} & & $\pm$7.4& & & & & & & \\ 
 {\bf33} & 8.06& 74$\pm$8& 2596$\pm$2& 128 137 144& 36.3& -17.10& 250& 2.3& \\ 
 {\bf34} & 4.17& 52$\pm$6& 1504$\pm$5& 89 102 106& 22.1& -14.84& 48& 3.6& \\ 
{\it35} & & $\pm$7.2& & & & & & & \\ 
&&&&& &&&&  \\  
{\it36} & & $\pm$12& & & & & & & \\  
 {\it37} & & $\pm$13& & & & & & & \\ 
 {\it38} & & $\pm$12& & & & & & & \\ 
 {\bf39} & 2.58& 59$\pm$10& 2043$\pm$4& 41 69 73& 30.0& -15.03& 55& 3.4& \\  
{\bf40} & 3.75& 47$\pm$7.9& 2492$\pm$3& 106 115 116& 36.1& -16.97& 120& 1.2&confused \\ 
&&&&& &&&& \\  
{\it41} & & $\pm$8& & & & & & &  \\  
 {\bf42} & 0.84& 29$\pm$5& 1510$\pm$7& 27 38 41& 23.4& -14.42& 11& 1.2& \\ 
 {\it43} & & $\pm$12& & & & & & & \\ 
 {\it44} & & $\pm$11& & & & & & & \\ 
 {\bf45} & 5.31& 81$\pm$10& 1435$\pm$2& 72 89 92& 21.5& -15.29& 58& 2.8& \\

&&&& &&&&& \\ 
\hline 
&&&&&&&\\
\multicolumn{10}{|l|}{         } \\  
\multicolumn{10}{|l|}{kkr\,3 = kk230 (e.g. Huchtmeier et. al 2000)   } \\  
\multicolumn{10}{|l|}{kkr\,40: UGC\,11111 (at 3.3') and UGC\,11113 (at
3.8') with similar radial velocities} \\  
\hline
\end{tabular}
\end{table*}
%\end{document} 
\begin{table*}
\begin{tabular}{|rccllclccl|} \hline
\multicolumn{1}{|r}{KKR}&  
\multicolumn{1}{c}{\HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{velocity}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{distance}&
\multicolumn{1}{c}{M$_{Bt}$}& 
\multicolumn{1}{c}{\HI mass}&   
%\multicolumn{1}{c}{total mass}& 
\multicolumn{1}{c}{M$_{\HI}$/L$_{B}$}& 
\multicolumn{1}{c|}{Comment}
\\ \hline   
\multicolumn{1}{|c}{No. }&
\multicolumn{1}{c}{Jy$\,$km$\,$s$^{-1}$}&
\multicolumn{1}{c}{mJy }&
\multicolumn{1}{c}{km$\,$s$^{-1}$}&
\multicolumn{1}{c}{km$\,$s$^{-1}$}&
\multicolumn{1}{c}{Mpc }&
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{10$^{7}$M$_{\odot}$}&
%\multicolumn{1}{c}{10$^{8}$M$_{\odot}$}& 
\multicolumn{1}{c}{  }&  
\multicolumn{1}{c|}{  }  
\\ \hline
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c|}{10} 
%\multicolumn{1}{c|}{11}
 \\ \hline  
 &&&&&& & & & \\
 46 & 3.53& 36$\pm$8.4& 3779$\pm$5& 50 127 130& 54.2& -16.77& 240& 3.1& \\ 
 47 & & $\pm$9.3& & & & & & & \\ 
 48 & 1.88& 30$\pm$7& 3158$\pm$3& 48 51 92& 45.9& -16.53& 94& 1.5& \\ 
 {\bf49} & 3.57& 55$\pm$8.2& 785$\pm$4& 72 91 99& 14.4& -15.78& 17& 0.6& \\ 
 {\it50} & & $\pm$11& & & & & & & \\ 
&&&&& &&&& \\  
51 & & $\pm$12& & & & & & & \\  
 {\it52} & & $\pm$18& & & & & & & \\ 
 {\it53} & & $\pm$12& & & & & & & \\ 
 54 & & $\pm$11& & & & & & & \\ 
55 & $\ge$1:&68 $\pm$9.3& 23:&$\ge$44: &5.4 &-14.8 &$\ge$0.7 &$\ge$0.07 &local
\HI?\\ 
&&&&& &&&& \\  
56 &5.6: &470 $\pm$8.5&-135: &10 22 24: &6.4 &-14.4 &5.4 &$\ge$0.56 &local
\HI\\ 
 57 & & $\pm$7.9& & & & & & & \\ 
 58 & 16.04& 101$\pm$9.4& 2756$\pm$2& 246 277 280& 40.7& -19.95& 630& 0.42& \\  
 59 &$\ge$36 &680 $\pm$8&$\le$17: &$\ge$64: &4.7 &-17.0 &$\ge$18.8 &$\ge$0.32 &local \HI? \\ 
60 & & $\pm$9.1& & & & & & & \\ 
&&&&& &&&& \\  
61 & 6.35& 110$\pm$8& 919$\pm$2& 74 81 90& 16.0& -14.82& 3.8& 2.9& \\  
 62 & & $\pm$18& & & & & & & \\  
 63 & & $\pm$8.1& & & & & & & \\ 
 64 & & $\pm$9.7& & & & & & & \\ 
65 & & $\pm$10& & & & & & & \\ 
&&&&& &&&& \\  
66 & & $\pm$7.8& & & & & & & \\ 
 67 & & $\pm$14& & & & & & & \\ 
 68 & 19.5& 291$\pm$7.4& 1145$\pm$1& 72 86 90& 19.2& -16.68& 170& 2.3&confused? \\ 
 69 & 14.3& 190$\pm$8.5& 1143$\pm$1& 74 90 94& 19.2& -15.24& 120& 6.4&confused\\  
70 & & $\pm$11& & & & & & & \\ 
&&&&& &&&& \\ 
71 & 5.64& 191$\pm$14& 693$\pm$2& 26 35 40& 13.1& -14.03& 23& 3.6& \\  
 72 & & $\pm$6.1& & & & & & & \\  
 73 & & $\pm$5.9& & & & & & & \\ 
 74 & & $\pm$6.4& & & & & & & \\ 
75 & 3.56& 38$\pm$4.3& 1469$\pm$5& 97 124 128& 22.4& -14.24& 42& 5.4& \\  
&&&&& &&&& \\ 
76 & & $\pm$7& & & & & & & \\ 
 77 & 0.45& 32$\pm$8.4& 3665$\pm$2& 29 33 40 & 51.7& -16.63& 28& 0.4& \\ 
 78 & & $\pm$6.9& & & & & & & \\ 
    &     &     &   &             & & & & &                    \\
\hline  
&&&&&&&\\
% &&&& &&&&& \\  
\multicolumn{10}{|l|}{kkr\,55, kkr\,56, kkr\,59 are possible companions of
NGC\,6946} \\  
\multicolumn{10}{|l|}{kkr\,69 within 4.1 arcmin from kkr\,68, confused  } \\  
\hline
% &&&&&& & & & \\
\end{tabular}
\end{table*}
\end{document}


