\begin{table}%t2 online %\centering \par \caption{\label{tab2}Comparison of previously published spectral classifications.} \begin{tabular}{lccccccc} \hline \hline \noalign{\smallskip} W\# & \multicolumn{7}{c}{Spectral classification} \\ & 1966 & 1973 & 1973-4? & 1981 & 1995 &2002 & 2006\\ \hline 4 &{\em OB}& {\em OB}&-- &G0 Ia & {\em OB} &F2 Ia & $<$G5 Ia \\ 6 &{\em OB}& -- &-- &B1 V & -- & B0.5 Iab & --\\ 7 &{\em OB}& {\em OB}&-- &A0 Ia & {\em OB} & B5 Ia & -- \\ 8a &{\em OB}& -- &-- &G0 Ia & {\em OB} & F5 Ia & $<$G5 Ia \\ 9 &{\em OB}& ? & ? &Be & {\em OB} & sgB[e] & $<$G5 Ia \\ 10 &{\em OB}& -- &-- &B0 III& -- & B0.5I+OB & --\\ 11 &{\em OB}& -- &-- &B1 II & -- & B2 Ia & --\\ 12a &{\em OB}&{\em OB} &-- &A2 Ia & {\em OB} & A5 Ia & $<$G5 Ia \\ 16a &{\em OB}&{\em OB} &-- &A2 Ia & {\em OB} & A2 Ia & --\\ 20 &{\em M} &{\em M} &{\em M} &M6 Ia & -- & $<$M6 I & M5 Ia\\ 26 &{\em M} &{\em M} &{\em M} &M2 Ia & {\em M} & $<$M6 I & M5-6Ia\\ 28 &{\em OB}& -- & -- &B0 II & -- &B2 Ia & -- \\ 31 &{\em OB}& -- & -- &Be & -- &B0I+OB & -- \\ 32 &{\em OB}&{\em OB} & -- &G5 Ia & {\em OB} &F5 Ia & $<$G5 Ia \\ 33 &{\em OB}& -- & -- &B8 Iab& {\em OB} &B5 Ia & --\\ 70 &{\em OB}& -- & -- &B8 Iab& -- & B3 Ia & -- \\ 71 &{\em OB}& -- & -- &B8 Iab& -- & B2.5 Ia & --\\ 75 &{\em M}&{\em M} &{\em M} &-- & -- & -- & M4 Ia\\ 78 &{\em OB}& -- &-- &B1~Ia & -- & B1 Ia & --\\ 237 &{\em M} &{\em M} &{\em M} &M6 & -- &$<$M6 I & M3 Ia\\ 243 &{\em OB}&{\em OB} &-- &B2Ia & -- &A2 Ia & --\\ 265 &{\em OB}&{\em OB} &-- &G0 Ia & -- &F5 Ia & $<$G5 Ia \\ \hline \end{tabular} \tablefoot{Note that classifications given in italics have been derived from photometric data alone, while the 2006 classifications are derived from 2.3~$\mu$m spectroscopy (Mengel \& \mbox{Tacconi-Garman} \cite{mengel}, \cite{mengel08}). Crowther et~al. (\cite{crowther}) provide a comparable table for the WR~population.} \vspace*{12mm} \end{table}