% TABLE1.TEX -- AASTeX sample table 1.

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\tablenum{1C}
\begin{planotable}{rccrrrrrrccrrl}
\tablewidth{0pc}
\tablecaption{Early-type stars, giants and degenerates}
\tablehead{
\colhead{ }           & \colhead{name}      &
\colhead{bin.}          & \colhead{}          & 
\colhead{$\alpha$}  &
\colhead{2000}          & \colhead{}    &
\colhead{$\delta$}  & \colhead{}  &
\colhead{Src.} & \colhead{V} & 
\colhead {M$_V$} &\colhead{r}  &
\colhead{Sp}}

\startdata

  176&GJ 1023 A &p&  0& 54& 18.4& 69&  2& 50&  3&   9.70&   4.4&   115& G0     \nl
  177&GJ 1023 B &s&  0& 54& 18.4& 69&  2& 50&  3&  10.40&   4.9&   125& G0     \nl
  183&G269-061  & &  0& 56& 19.5&-28&  8& 21&  3&  10.96&   6.7&    70& K3     \nl
  185&Gl  44    & &  0& 57& 20.2& -1& 48& 56&  3&   9.46&   6.2&    45& K1     \nl
  188&GJ 2017   & &  0& 59& 51.5&-25& 35& 25&  3&   9.87&   4.1&   145& G0     \nl
  192&GJ 2019   & &  1&  0& 37.0&-26& 38& 15&  3&  10.11&   5.6&    80& G5     \nl
  198&GJ 2020   & &  1&  1& 49.2&-25& 53& 12&  3&   9.75&   2.9&   230& F2     \nl
  201&RGO 2913   & &  1&  1& 54.2&-25& 45& 38&  3&  11.84&   7.8&    65& K5     \nl
  228&Gl  53.3  & &  1&  9& 43.4& 35& 37& 15&  4&   2.05&   0.5&    20\tablenotemark{a}& M0 III \nl
  306&BD+63 219 & &  1& 41&  9.9& 63& 48& 43&  3&  10.07&   3.9&   175& A5     \nl
  387&Rob 115   & &  2& 10& 13.4& 11& 31& 58&  3&  12.72&  -0.8&  5000\tablenotemark{b}& M4 III \nl
  579& AC +0:641-15& &  3& 14& 20.3&  0& 39& 11&  3&   9.40&   6.7&    35\tablenotemark{b}& G3     \nl
  602&LP355-65  &s&  3& 22& 52.7& 27&  8& 44&  2&  18.00&  15.6&    30\tablenotemark{c}& DC     \nl
  666&Wo 9124   & &  3& 44& 20.0& 24& 47& 45&  3&  10.66&   5.1&   130& K1     \nl
  667&Wo 9125   & &  3& 44& 20.4& 24& 46& 21&  3&  10.81&   5.3&   125& K5     \nl
  669&Wo 9127   & &  3& 44& 22.1& 24& 45& 57&  4&  11.09&   6.2&    95& G0     \nl
  720&Gl 160.2  & &  4&  6& 34.7&-20& 51&  0&  3&   9.68&   7.7&    25& K4     \nl
  755&Gl 168.1  & &  4& 22& 10.3& 19& 28& 59&  3&  15.04&   4.8&   450& G0\tablenotemark{d}   \nl
  757&LH190     & &  4& 22& 16.5& 15& 30& 44&  2&  17.00&   9.0&   100\tablenotemark{b}& M1?\tablenotemark{d}   \nl
  763&vA342      & &  4& 25&  0.2& 16& 59&  4&  3&  10.31&   7.0&    45& K3     \nl
  820&AC+19:1513-210 & &  4& 43& 26.5& 19&  0& 18&  3&  13.40&   6.5&   240\tablenotemark{b}& G0     \nl
  909&GJ 2040   & &  5& 19& 34.9&  3& 52& 24&  3&   9.86&   7.9&    25& K0     \nl
  985&Gl 223.1  & &  5& 54& 34.0& -9& 23& 34&  3&  10.71&   7.7&    40& K4     \nl
 1306&V518      & &  8& 18& 44.3&-15& 12&  7&  3&   9.84&   7.5&    30& K3     \nl
 1314&Gl 305.1  & &  8& 23& 30.7& 21& 50& 58&  3&   9.54&   7.6&    25& K3     \nl
 1354&GJ 1113   & &  8& 40& 36.7& 43&  6& 51&  3&   9.32&   7.3&    25& K2     \nl
 1384&GJ 1115   & &  8& 53& 47.3& 35& 13& 21&  3&   9.30&   7.8&    20& K3     \nl
 1418&GJ 1120 A &p&  9&  1& 17.5& 15& 15& 57&  3&   9.43&   7.9&    20& K4     \nl
 1597&Gl 383.1  & & 10& 13& 57.3& 52& 30& 28&  3&   9.53&   7.5&    25& K2     \nl
 1689&Gl 402.1  & & 10& 52&  2.6&  0& -9& 35&  3&  10.20&   6.3&    60& K0     \nl
 1714&Gl 409    & & 11&  1& 57.2&-17& 57& 23&  3&  11.87&   4.8&   265& G5     \nl
 1885&Gl 454.1  & & 12&  1&  7.2& -1& 43& 54&  3&  10.96&   7.5&    50& K3     \nl
 1912&Wo 9394   & & 12& 12&  1.4& 13& 15& 43&  3&  10.18&   3.9&   180& F2     \nl
 2034&Gl 489    & & 12& 57& 44.0&-14& 27& 47&  3&   9.12&   7.6&    20& K3     \nl
 2053&Gl 499.1  & & 13&  6& 22.5& 22& 36& 56&  3&   5.60&   0.0&   130\tablenotemark{e}& M5 III \nl
 2149&Gl 518.2B &s& 13& 37& 13.8& 30&  5& 12&  3&  10.51&   6.0&    80& K1     \nl
 2197&GJ 1180   & & 13& 51& 59.5& 26& 38& 10&  3&  10.83&   5.5&   115& G5     \nl
 2213&LTT 5453   & & 13& 59&  7.6&-23& 33& 28&  4&  14.93&  14.7&    11\tablenotemark{f}& DA     \nl
 2287&Gl 550.1  & & 14& 27& 45.3& 23& 50& 26&  3&  10.92&   7.9&    40& K4     \nl
 2328&Gl 561    & & 14& 43& 19.2& 26& 44& 58&  3&   9.67&   5.4&    70& K0     \nl
 2335&Gl 562    & & 14& 46& 23.3& 16& 29& 55&  3&   9.25&   8.4&    15& K4     \nl
 2347&LTT 14398 &s& 14& 51&  2.3&  9& 43& 23&  3&   8.90&   7.1&    23\tablenotemark{c}& K4     \nl
 2609&Gl 629.2A &p& 16& 34& 42.3& -4& 13& 39&  3&   9.62&   5.6&    65& F8     \nl
 2656&BD+38 2847 & & 16& 50& 54.2& 38&  9&  0&  3&  10.55&   7.1&    50\tablenotemark{b}& K3     \nl
 2759&AC+02:2142-173& & 17& 26& 10.6&  1& 48& 20&  3&  10.90&   5.1&   145& G0     \nl
 2768&Gl 677  A &p& 17& 29& 20.1& 29& 23& 32&  3&   9.55&   7.6&    25& K3     \nl
 2807&Gl 690  A &p& 17& 38& 33.9& 71& 19& 53&  3&   9.20&   7.2&    25& K4     \nl
 2856&Gl 700.1C &s& 18&  3& 13.9& -8& 11& 25&  1&   9.40&   5.9&    50\tablenotemark{b}& G1     \nl
\phantom{0} 3022&LP336-6   & & 19& 11&  5.9& 32& 39& 59&  3&  10.48&   0.5&  1000\tablenotemark{b}& M0 III \nl
 3030&Gl 748.2A &p& 19& 14& 58.6&  2&  9& 47&  3&  10.20&   7.8&    30& K2     \nl
 3309&Wo 9723   & & 21&  8& 44.0& 47&  9&  8&  1&  10.78&   6.6&    70& K2     \nl
 3315&GJ 2152   & & 21& 13& 29.1&  7& 26& 13&  4&  16.17&  16.0&    11\tablenotemark{f}& DA     \nl
 3438&BD+32 4292A &p& 21& 55& 38.6& 33&  2& 11&  3&  10.00&   5.0&   100\tablenotemark{b}& G0     \nl
 3462&AC+01:2189-92& & 22&  3& 28.6&  1& 35& 48&  3&  10.34&   5.5&    95& K1     \nl
 3493&Wo 9775   & & 22& 14& 24.0& -8& 44& 38&  3&  11.85&   6.0&   150\tablenotemark{b}& K1     \nl
 3495&Gl 851.4  & & 22& 14&  0.9& 57&  7& 12&  3&   9.83&   5.5&    75& K0     \nl
 3555&VVO 271    & & 22& 37& 11.9&  0&-39&  1&  3&  10.50&   6.0&    80\tablenotemark{b}& G8     \nl
 3585&BD+43 4306  & & 22& 47& 31.6& 44& 33& 11&  3&   9.60&   3.7&   150\tablenotemark{b}& G0     \nl
 3692&Wo 9826   & & 23& 25& 55.3& 29& 11& 42&  3&  11.05&   6.5&    80& K1     \nl
 3734&LP463-28  &s& 23& 38& 58.6& 21&  1& 23&  2&  16.40&  14.3&    26\tablenotemark{c}& DC     \nl
 3798&Wo 9848   & &  0&  1& 54.4& 26&  0& 38&  1&  11.30&   6.5&    90& K0     \nl
\tablenotetext{a} {distance from CNS3;}
\tablenotetext{b} {distance estimated from the spectral type;}
\tablenotetext{c} {distance estimated from companion star;}
\tablenotetext{d} {757: foreground reddening probably present;}
\tablenotetext{e} {FS Comae - distance based on Jura \& Kleinmann's M$_K$;}
\tablenotetext{f} {distance from McCook \& Sion (M$_V$, B-V) relations}

\tablecomments{V magnitudes are from the CNS3; absolute magnitudes are derived 
using Reid \& Murray's (1991) (M$_V$, (B-V)) relation unless otherwise indicated.}
\end{planotable}

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