\documentstyle{l-aa} \begin{document} \setcounter{table}{2} \begin{table} \caption{CORAVEL and ELODIE vsini measurements of Pleiades stars from the Hertzsprung and Soderblom samples} \begin{tabular}{llll|llll|llll} \hline \noalign{\smallskip} \multicolumn{1}{l}{star} & \multicolumn{1}{l}{\footnotesize {B--V}$_0$} & \multicolumn{2}{c}{{$v\sin i$}~ ({km\,s$^{-1}$})} & \multicolumn{1}{l}{star} & \multicolumn{1}{l}{\footnotesize {B--V}$_0$} & \multicolumn{2}{c}{{$v\sin i$}~ ({\,km\,s$^{-1}$})} & \multicolumn{1}{l}{star} & \multicolumn{1}{l}{\footnotesize {B--V}$_0$} & \multicolumn{2}{c}{{$v\sin i$}~ ({km\,s$^{-1}$})} \\ \multicolumn{1}{l}{HII} & \multicolumn{1}{l}{} & \multicolumn{1}{l}{\scriptsize CORAVEL} & \multicolumn{1}{l}{\scriptsize ELODIE} & \multicolumn{1}{l}{HII} & \multicolumn{1}{l}{} & \multicolumn{1}{l}{\scriptsize CORAVEL} & \multicolumn{1}{l}{\scriptsize ELODIE} & \multicolumn{1}{l}{HII} & \multicolumn{1}{l}{} & \multicolumn{1}{l}{\scriptsize CORAVEL} & \multicolumn{1}{l}{\scriptsize ELODIE}\\ \noalign{\smallskip} \hline 25 &0.443 &44.2$\pm$4.9 & & 793 &1.378 & &5.0$\pm$0.8& 1593 &0.716 &3.0$\pm$1.4 &1.8$\pm$1.0 \\ 34 &0.888 &7.3$\pm$1.1 &5.9$\pm$0.8 & 799 &1.287 & &4.7$\pm$0.8 & 1613 &0.494 &20.1$\pm$0.8 &\\ 97 &1.043 & &6.8$\pm$0.8& 870 &0.68 & &9.7$\pm$0.9 & 1726 &0.505 &12.9$\pm$0.7 & \\ 102 &0.684 &18.3$\pm$0.5 & & 879 &1.032 &7.2$\pm$1.3 &5.6$\pm$0.8& 1756 &1.325 & &5.0$\pm$0.8 \\ 120 &0.666 &9.4$\pm$1.2 & & 882 &1.040 &no dip & & 1766 &0.435 &22.7$\pm$1.3 &\\ 129 &0.830 &5.3$\pm$1.4 && 883 &1.086 & &3.8$\pm$0.8 & 1776 &0.680 &10.3$\pm$1.0 &9.8$\pm$0.9 \\ 152 &0.647 &11.1$\pm$1.2 &11.8$\pm$0.9 & 885 &0.988 &6.1$\pm$1.1 &5.2$\pm$0.8& 1785 &1.361 & &6.5$\pm$0.8 \\ 164 &0.459 &38.9$\pm$5.1 & & 890 &1.344 & &5.4$\pm$0.8 & 1794 &0.589 &11.2$\pm$0.8 &\\ 173{\footnotesize a} &0.73 &7.8$\pm$1.2 && 915 &1.199 & &9.3$\pm$0.8 & 1797 &0.515 &19.6$\pm$0.9 & \\ 173{\footnotesize b} &0.83 &6.3$\pm$2.2 & & 916 &0.824 &6.7$\pm$1.0 &5.6$\pm$0.8& 1856 &0.514 &15.4$\pm$0.9 & \\ 174 &0.811 &no dip & & 923 &0.579 &18.2$\pm$0.6 & & 1924 &0.568 &14.2$\pm$0.7 &\\ 186 &0.76 &11.1$\pm$0.7 && 974 &1.288 & &4.2$\pm$0.8 & 2016 &1.181 & &9.8$\pm$0.9 \\ 189 &1.328 & &4.7$\pm$0.8 & 996 &0.603 &11.9$\pm$0.8 && 2027{\footnotesize a} &0.76 &5.6$\pm$1.6 & \\ 191 &1.36 & &9.1$\pm$0.8 & 1015 &0.609 &9.6$\pm$1.1 & & 2106 &0.823 &3.7$\pm$1.5 &8.0$\pm$0.8\\ 193 &0.758 &6.3$\pm$1.4 &6.8$\pm$0.8& 1032 &0.733 &37.2$\pm$1.9 & & 2126 &0.815 &2.6$\pm$1.7 &5.3$\pm$0.8 \\ 233 &0.493 &14.1$\pm$0.7 & & 1039 &0.958 &$<$ 5 &4.9$\pm$0.8& 2147{\footnotesize a} &0.742 &6.9$\pm$3.2 & \\ 248 &0.738 &12.1$\pm$1.1 & & 1061 &1.358 & &7.1$\pm$0.8 & 2147{\footnotesize b} &0.742 &10.8$\pm$2.3 &\\ 250 &0.637 &6.9$\pm$1.1 &5.9$\pm$0.8& 1095 &0.858 &3.6$\pm$2.6 &3.6$\pm$0.8 & 2172 &0.582 &10.3$\pm$0.4 & \\ 253 &0.648 &38.2$\pm$1.8 & & 1100 &1.088 & &5.4$\pm$0.8& 2209 &1.336 & &5.4$\pm$0.8 \\ 263 &0.836 &7.8$\pm$0.8 & & 1101 &0.572 &SB2 & & 2278 &0.828 &6.1$\pm$0.9 &7.7$\pm$0.8\\ 293 &0.665 &6.6$\pm$1.0 &5.1$\pm$0.8& 1110 &1.170 & &5.9$\pm$0.8 & 2284 &0.743 &3.5$\pm$1.3 &3.7$\pm$0.8 \\ 296 &0.799 &14.7$\pm$0.9 & & 1114 &1.357 & &7.3$\pm$0.8& 2311 &0.780 &6.2$\pm$1.3 &6.5$\pm$0.8 \\ 298 &0.835 &6.6$\pm$1.1 &6.3$\pm$0.8 & 1117{\footnotesize a} &0.62 &6.4$\pm$2.6 & & 2341 &0.672 &3.4$\pm$1.7 &3.6$\pm$0.8\\ 303 &0.856 &17.4$\pm$0.7 && 1117{\footnotesize b} &0.67 &3.6$\pm$2.5 & & 2366 &0.779 &2.9$\pm$1.7 &4.3$\pm$0.8 \\ 314 &0.613 &41.9$\pm$1.6 & & 1122 &0.425 &28.6$\pm$1.2 && 2406 &0.720 &9.2$\pm$0.5 &8.5$\pm$0.8 \\ 320 &0.840 &10.8$\pm$0.5 & & 1124 &0.924 &5.6$\pm$3.3 &3.5$\pm$0.8 & 2407$^\dagger$ &0.910 & &6.3$\pm$0.8\\ 338 &0.428 &$>$40 && 1132 &0.451 &$>$40 & & 2462 &0.791 &5.4$\pm$1.2 &4.9$\pm$0.8 \\ 345 &0.806 &18.9$\pm$0.7 & & 1136 &0.784 &no dip && 2500 &0.58 &33.0$\pm$3.4 & \\ 357 &1.182 & &10.0$\pm$0.9 & 1139 &0.437 &31.4$\pm$1.9 & & 2506 &0.552 &13.8$\pm$0.8 &\\ 380 &1.171 & &6.0$\pm$0.8& 1182 &0.597 &16.4$\pm$1.1 & & 2548 &1.297 & &5.7$\pm$0.8 \\ 405 &0.495 &18.2$\pm$1.0 & & 1200 &0.507 &13.7$\pm$0.9 && 2588 &1.133 & &5.2$\pm$0.8 \\ 430 &0.777 &7.3$\pm$1.0 &6.3$\pm$0.8 & 1207 &0.591 &5.1$\pm$1.3 & & 2644 &0.698 &3.6$\pm$1.9 &5.0$\pm$0.8\\ 451 &1.169 & &5.7$\pm$0.8& 1215 &0.599 &6.5$\pm$0.9 &4.1$\pm$0.8 & 2665 &0.790 &5.9$\pm$1.2 &5.4$\pm$0.8 \\ 476 &0.53 &21.0$\pm$1.0 & & 1220 &0.830 &4.8$\pm$1.3 &6.3$\pm$0.8& 2741 &0.972 & &7.8$\pm$0.8 \\ 489 &0.594 &18.3$\pm$0.8 & & 1275 &0.791 &6.4$\pm$1.2 &6.4$\pm$0.8 & 2786 &0.562 &22.0$\pm$1.0 &\\ 513 &1.275 & &7.4$\pm$0.8& 1298 &0.957 &5.6$\pm$2.2 &4.8$\pm$0.8 & 2870 &0.974 & &4.0$\pm$0.8 \\ 514 &0.657 &10.5$\pm$1.0 & & 1332 &0.988 &$<$ 2 &5.3$\pm$0.8& 2880 &0.818 &6.3$\pm$1.1 &6.0$\pm$0.8 \\ 522 &0.879 &3.6$\pm$0.8 &4.4$\pm$0.8 & 1348{\footnotesize a} &1.05 & &5.1$\pm$0.8 & 2881$^\star$ &0.920 &7.8$\pm$1.1 &13.3$\pm$1.0\\ 571 &0.748 &7.6$\pm$0.5 &6.8$\pm$0.8& 1348{\footnotesize b} &1.35 & &1.8$\pm$0.8 & 2984 &0.961 & &5.4$\pm$0.8 \\ 590 &1.323 & &6.9$\pm$0.8 & 1355 &1.362 & &12.5$\pm$0.9& 3019 &1.174 & &6.0$\pm$0.8 \\ 627 &0.473 &33.2$\pm$1.3 & & 1392 &0.55 &15.7$\pm$1.6 & & 3096 &0.948 &6.2$\pm$1.3 &\\ 636 &0.981 & &3.5$\pm$0.8& 1454 &1.068 & &3.3$\pm$0.8 & 3097 &0.697 &14.6$\pm$0.3 & \\ 659 &0.66 &12.2$\pm$1.1 & & 1485 &1.309 & &42.0$\pm$2.2& 3104 &1.24 & &7.1$\pm$0.8 \\ 676 &1.065 & &5.5$\pm$0.8 & 1512 &1.207 & &5.3$\pm$0.8 & 3179 &0.529 &5.5$\pm$1.2 &4.3$\pm$0.8\\ 727 &0.519 &$>$40 && 1514 &0.609 &13.6$\pm$0.8 & & 3187 &1.139 & &6.2$\pm$0.8 \\ 739 &0.586 &14.4$\pm$0.6 & & 1516 &1.267 & &105$\pm$10& &&&\\ 746 &0.768 &4.9$\pm$1.0 &4.8$\pm$0.8 & 1553 &1.078 & &9.6$\pm$0.9 & &&&\\ \hline \end{tabular} \end{table} \clearpage \begin{table} \caption{ CORAVEL vsini measurement of stars located in the corona of the Pleiades and recently selected by Rosvick et al. and by Mermilliod et al. as cluster members} \begin{tabular}{lll|lll|lll} \hline \noalign{\smallskip} \multicolumn{1}{l}{star} & \multicolumn{1}{l}{{(B$-$V)$_{0}$}} & \multicolumn{1}{l}{ {$v\sin i$}~({\,km\,s$^{-1}$})} & \multicolumn{1}{l}{star} & \multicolumn{1}{l}{{(B$-$V)$_{0}$}} & \multicolumn{1}{l}{ {$v\sin i$}~({\,km\,s$^{-1}$})} & \multicolumn{1}{l}{star} & \multicolumn{1}{l}{{(B$-$V)$_{0}$}} & \multicolumn{1}{l}{ {$v\sin i$}~({\,km\,s$^{-1}$})}\\ \noalign{\smallskip} \hline R60 &0.440 &no dip & Pels 39$^\star$ &0.83 &2.0$\pm$2.0 & Pels 143 &0.85 &5.2$\pm$1.2 \\ S151x &0.46 &21.6$\pm$1.0 & Pels 40 &0.53 &11.9$\pm$0.7& Pels 146 &0.62 &17.6$\pm$1.4 \\ S183x &0.5 &32.3$\pm$1.4& Pels 44 &0.86 &3.9$\pm$3.1 & Pels 150 &0.48 &26.3$\pm$1.7 \\ S37 &0.403 &no dip & Pels 45 &0.78 &7.8$\pm$1.3 & Pels 151 &0.67 &5.5$\pm$2.2 \\ S39 &0.424 &no dip & Pels 46 &0.7 &8.1$\pm$1.2& Pels 173 &0.41 &36.7$\pm$3.0 \\ Pels 3 &0.47 &SB2& Pels 47 &0.86 &4.5$\pm$1.5 & Pels 174 &0.54 &$>$40 \\ Pels 4 &0.78 &2.6$\pm$1.7 & Pels 50 &0.8 &7.0$\pm$1.5 & Ia 317 &0.5 &$>$40 \\ Pels 5 &0.66 &11.1$\pm$0.9 & Pels 56 &0.77 &$>$40& Ib 038 &0.66 &10.9$\pm$0.9 \\ Pels 6 &0.47 &35.9$\pm$3.1& Pels 60 &0.52 &no dip & Ib 055 &0.74 &6.6$\pm$1.0 \\ Pels 7 &0.62 &2.7$\pm$1.9 & Pels 68 &0.81 &6.7$\pm$2.0 & Ib 078 &1.03 &6.4$\pm$1.1 \\ Pels 8 &0.64 &15.5$\pm$1.0 & Pels 69 &0.81 &16.3$\pm$0.8& Ib 146a &0.45 &12.4$\pm$3.5 \\ Pels 11 &0.82 &5.2$\pm$1.3& Pels 71 &0.77 &9.1$\pm$1.1 & Ib 146b &0.5 &8.6$\pm$5.3 \\ Pels 12 &0.69 &11.2$\pm$0.9 & Pels 75 &0.87 &$>$40 & Ib 288 &1.01 &SB2 \\ Pels 15 &0.54 &24.4$\pm$1.1 & Pels 78 &0.7 &8.8$\pm$1.1& II 293 &0.65 &8.5$\pm$0.9 \\ Pels 17 &0.5 &29.3$\pm$2.0& Pels 79 &0.73 &2.8$\pm$1.7 & II 359 &0.57 &16.6$\pm$0.9 \\ Pels 18 &0.58 &11.8$\pm$1.0 & Pels 83 &0.69 &14.5$\pm$1.1 & III 059 &0.8 &4.1$\pm$1.2 \\ Pels 19 &0.85 &4.8$\pm$1.4 & Pels 86 &0.45 &no dip& III 079 &0.43 &no dip \\ Pels 20 &0.61 &9.6$\pm$1.1& Pels 89 &0.84 &3.2$\pm$2.1 & III 391 &0.73 &2.3$\pm$1.8 \\ Pels 23 &0.55 &36.2$\pm$1.7 & Pels 121 &0.62 &4.9$\pm$1.1 & III 679 &0.96 &4.1$\pm$1.5 \\ Pels 25 &0.443 &no dip & Pels 123 &0.92 &3.1$\pm$2.1& III 700 &0.67 &9.3$\pm$0.9 \\ Pels 28 &0.94 &8.9$\pm$1.2& Pels 124 &0.5 &20.5$\pm$0.9 & IV 131 &0.77 &2.2$\pm$1.5 \\ Pels 29 &0.6 &33.8$\pm$1.9 & Pels 126 &0.58 &9.8$\pm$1.0 & IV 314 &0.98 &2.7$\pm$2.8 \\ Pels 30 &0.9 &6.7$\pm$1.1 & Pels 128 &0.61 &4.6$\pm$1.5& V 088 &0.77 &5.2$\pm$1.2 \\ Pels 31 &0.94 &12.2$\pm$1.0& Pels 135 &0.45 &no dip & V 198a &0.6 &10.5$\pm$1.1 \\ Pels 34 &0.69 &3.6$\pm$1.4 & Pels 137 &1.01 &3.6$\pm$1.6 & V 198b &0.87 &2.0$\pm$2.0 \\ Pels 35 &0.51 &19.4$\pm$1.1 & Pels 138 &0.76 &5.6$\pm$1.6& V 308 &0.78 &8.0$\pm$1.0 \\ Pels 37 &0.63 &13.4$\pm$2.6& Pels 140 &0.45 &11.5$\pm$1.2 & && \\ Pels 38 &0.73 &3.1$\pm$2.0 & Pels 142 &0.81 &3.9$\pm$1.5 & &&\\ \hline \end{tabular} \end{table} \clearpage \begin{table} \caption{ELODIE vsini and radial velocity measurements of new members of the Pleiades corona} \begin{tabular}{llllr|llllr} \hline \noalign{\smallskip} \multicolumn{1}{l}{star} & \multicolumn{1}{l}{{(B$-$V)$_{0}$}} & \multicolumn{1}{l}{ {$v\sin i$}} & \multicolumn{1}{l}{$V_r$} & \multicolumn{1}{l}{($O-C$)}&\multicolumn{1}{l}{star} & \multicolumn{1}{l}{{(B$-$V)$_{0}$}} & \multicolumn{1}{l}{ {$v\sin i$}} & \multicolumn{1}{l}{$V_r$} & \multicolumn{1}{l}{($O-C$)}\\ \noalign{\smallskip} \hline Pels 9 &1.0 &5.5$\pm$0.8 &6.41 &$-0.15$ & Pels 72 &0.72 &160$\pm$10 &6.0: &0.78 \\ Pels 22 &0.90 &12.1$\pm$0.9 &5.08 &0.34& Pels 109 &1.31 &5.5$\pm$0.8 &4.96 &$-0.35$ \\ Pels 41 &0.90 &5.1$\pm$0.8 &5.59 &0.56 & Pels 114 &1.04 &6.0$\pm$0.8 &6.70 &0.21 \\ Pels 43 &0.92 &6.8$\pm$0.8 &4.92 &0.04& Pels 115 &1.06 &5.5$\pm$0.8 &6.28 &0.24 \\ Pels 59 &0.99 &5.6$\pm$0.8 &5.06 &0.02 & Pels 137 &1.01 &5.2$\pm$0.8 &4.90 &0.12 \\ Pels 63 &1.07 &2.9$\pm$0.8 &7.41 &$-0.36$& Pels 162 &0.91 &3.2$\pm$0.8 &6.10 &$-0.18$ \\ Pels 66 &1.0 &4.9$\pm$0.8 &7.39 &0.45 & Pels 189 &0.93 &4.9$\pm$0.8 &5.87 &0.53 \\ Pels 71 &0.77 &11.1$\pm$0.9 &6.25 &0.23& Pels 192 &1.34 &11.4$\pm$0.9 &6.77 &0.34 \\ \hline \end{tabular} \end{table} \end{document}