Table 1: The distribution of stars over main-sequence spectral type for the Kroupa and Salpeter mass distributions (BD = brown dwarfs).
\begin{displaymath}\begin{tabular}{l r@{$-$}l r@{.}l r@{.}l r@{.}l r@{.}l} \hli... ...& 100&00 & 100&00 & 100&00 & 100&00 \\ \hline \end{tabular}\end{displaymath}


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