% TABLE1.TEX -- AASTeX sample table 1.

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\tablenum{1D}
\begin{planotable}{lcrrrrrrccrrrlrl}
\tablewidth{0pc}
\tablecaption{Additional stars}
\tablehead{
 \colhead{name}      & \colhead{} &
\colhead{}          & \colhead{$\alpha$}  &
\colhead{2000}          & \colhead{}    &
\colhead{$\delta$}  & \colhead{}  &
\colhead{Src.} & \colhead{M$_V$} &
\colhead{r}  & \colhead{$\epsilon_r$}  &
\colhead{dist.}  & \colhead{$V_r$}  &
\colhead{Sp}}

\startdata
 RE0618+75 & &  6& 18& 10.2& 75&  6& 49&  3&   9.99&  21.0&  30&Sp & -28.3 &  M 1.5 \nl
 GJ 1285& & 23& 31&  7.5& -2& 45&  0&  3&  13.66&  29.2&  9&$\pi$ & -19.8&  M 4.5 \nl
  Gl 129   & &  3& 13& 44.7& 18& 50& 37&  2&  11.70&  32.4&   8&$\pi$ &-105.8 & K 5\tablenotemark{c}  \nl
  LP855-60\tablenotemark{d} & & 13& 44&  0.0&-26& 18&  0&  3&  12.10&  19.1&  29&Sp &-42.9&  M 3.5 \nl
BRI0021-0214\tablenotemark{e}& &  0& 24& 21.4&-2& 31& 29&  2&  18.31&  13.8&   3&$\pi$ & 16.0&  M 9.5
\tablenotemark{f}   \nl

\tablenotetext{a}{from Jefferies et al, 1993 - binary system}
\tablenotetext{b}{Bond's flare star from Greenstein, 1977}
\tablenotetext{c}{Strong CaH - probable halo subdwarf}
\tablenotetext{d}{from Brosch \& Goldberg, 1994}
\tablenotetext{e}{from Irwin et al, 1991}
\tablenotetext{f}{spectral type from Kirkpatrick et al, 1995}
\tablecomments{
dist - indicates whether the distance estimate is based on a 
trigonometric parallax measurement or on our spectroscopic data; \nl
$V_r$ - the radial velocity derive from our spectroscopy.}
\end{planotable}

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