\begin{table}%t5
\caption{This table was organized in increasing order of $T\rm _{eff}$, with the
comments about the results shown in the last column of each series of 4~columns.
\label{comm}}
 \begin{tabular}{lcll|clcll|clcll}
\hline\hline
%\noalign{\smallskip}
Star & $T\rm _{eff}$(K) & $\log g$ & Comm. && Star & $T\rm _{eff}$(K) & $\log g$ & Comm.  && Star & $T\rm _{eff}$(K) & $\log g$ & Comm.\\
%\noalign{\smallskip}
\hline
HD 123396  & 4360 & 1.4(3)  &         && HD 202109  & 4910 & 2.41    &      && HD 13551   & 5870 & 4.0(1)  &  \\
HD 220009  & 4370 & 1.91    &         && HD 104979  & 4920 & 2.58    &      && HD 106191  & 5890 & 4.2(1)  & a, c, g \\
HD 210910  & 4570 & 2.7(2)  & a, b, f && HD 46407   & 4940 & 2.65    &      && HD 8270    & 5940 & 4.2(1)  &  \\
HD 5424    & 4570 & 2.0(3)  &         && HD 223938  & 4970 & 3.1(1)  &      && HD 147609  & 5960 & 4.42(9) & a, b, e \\
HD 749     & 4610 & 2.8(1)  &         && HD 12392   & 5000 & 3.2(1)  &      && HD 89948   & 6010 & 4.30(8) & h \\
HD 210709  & 4630 & 2.4(2)  &         && HD 139195  & 5010 & 2.89    &      && HD 188985  & 6090 & 4.3(1)  & c \\
HD 26967   & 4650 & 2.51    &         && HD 20894   & 5080 & 2.60    & j    && HD 76225   & 6110 & 3.8(1)  & i \\
HD 116869  & 4720 & 2.2(2)  &         && HD 113226  & 5082 & 2.85    &      && HD 222349  & 6130 & 3.9(1)  &  \\
HD 205011  & 4780 & 2.41    &         && HD 13611   & 5120 & 2.49    &      && HD 92545   & 6210 & 4.0(1)  & c \\
HD 9362    & 4780 & 2.43    &         && HD 204075  & 5250 & 1.53    & c, f && BD+18 5215 & 6300 & 4.2(1)  & d \\
HD 116713  & 4790 & 2.67    &         && HD 22589   & 5400 & 3.3(1)  &      && HD 150862  & 6310 & 4.6(1)  & c \\
HD 181053  & 4810 & 2.48    &         && HD 87080   & 5460 & 3.7(2)  &      && HD 107574  & 6400 & 3.6(2)  & c \\
HD 27271   & 4830 & 2.9(1)  &         && HD 48565   & 5860 & 4.01(8) & i    && HR 107     & 6440 & 4.08(7) & a, b \\
\hline
\end{tabular}
 \par
Comments: a. upper limit for Hf; b. one of the lines has only an
upper limit for Ru; c. poor line profiles at~$\lambda$4080; d. poor
line profiles of \ion{Ru}{i} at~$\lambda$4757; e. poor line profile
of \ion{Hf}{ii} at $\lambda$4093; f. very broadened spectral
lines; g. $S/N$~$\approx$~100; h. $S/N$~$\approx$~250; i. $\Delta$(Ru) $>$
0.3; j. $\Delta$(Hf) $>$ 0.3.
\end{table}