\begin{table}%t5
  \caption{Properties of the IRAS FIR~flux limited sample of Abell~262  galaxies with a distance to the cluster core of less than~3~Abell radii, as observed in HI~by \citeauthor{1985apj...292..404g}.  The morphological classification, as well as the inclination estimate (with respect to the line of sight), were taken from 
  \citet{1973UGC...C...0000N}, $D_{25}$ from \citet{1991trcb.book.....D},
  $S_{60~\mu \rm{m}}$ and $S_{100~\mu \rm{m}}$ IRAS flux densities from
  \citet{1990irasf.c......0m}, and HI~deficiency from
  \citet{1985apj...292..404g}. An inclination value of 1 indicates a face-on, and a 7 indicates an edge-on view onto the galaxy.} 
  %\centering
\par
  \begin{tabular}{ccccccccccc}
     \hline
     \hline
  \multicolumn{1}{c}{Obj.} &   \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{Incl.} &\multicolumn{1}{c}{$D_{25}$}  &\multicolumn{1}{c}{$S_{12~\mu \rm{m}}$}  &\multicolumn{1}{c}{$S_{25~\mu \rm{m}}$} &\multicolumn{1}{c}{$S_{60~\mu \rm{m}}$} &\multicolumn{1}{c}{$S_{100~\mu \rm{m}}$} &\multicolumn{1}{c}{$L_{\rm{FIR}}$}             & \multicolumn{1}{c}{HI}        & \multicolumn{1}{c}{$r/r_A$} \\ 
                           &                             &  class                         &\multicolumn{1}{c}{[\arcmin]} &\multicolumn{1}{c}{[Jy]}                &\multicolumn{1}{c}{[Jy]}               &\multicolumn{1}{c}{[Jy]}               &\multicolumn{1}{c}{[Jy]}                &\multicolumn{1}{c}{[10$^9 h^{-2}~L_{\odot}$]} & \multicolumn{1}{c}{deficiency}&                             \\
      \hline
  UGC 1048 &  SBa      & 1  &  1.58 & 0.14& 0.47  & 3.75 &  6.95  &   15.76 &   0.2 & 3.07\\
  UGC 1089 &  Sc       & 1  &  1.15 & 0.12& 0.19  & 1.08 &  3.17  &    5.65 &  0.14 & 2.88\\
  UGC 1094 &  SBb      & 6  &  2.24 & 0.11& 0.16  & 1.03 &  3.19  &    5.55 &  0.07 & 2.9\\
  UGC 1100 &  Sb/SBb   & 6  &  2.19 &$<$0.11&$<$0.08  & 0.25 &  1.02  &    1.57 &  0.29 & 2.41\\
  UGC 1125 &  S        &    &       &$<$0.08&$<$0.12  & 0.42 &  1.05  &    2.02 &  --0.2 & 2.44\\
  UGC 1152 &  Sb       & 5  &  1.05 &$<$0.08&$<$0.10  & 0.32 &  0.79  &    1.53 & --0.12 & 3.05\\
  UGC 1178 &  Sc       & 7  &  1.82 & 0.14& 0.12  & 1.23 &  3.66  &    6.48 & --0.27 & 1.69\\
  UGC 1220 &  S        &    &  0.83 & 0.14& 0.26  & 1.88 &   4.6  &    8.95 &     0 & 1.3\\
  UGC 1234 &  Sc/SBc   &    &  1.12 &$<$0.07&$<$0.09  & 0.23 &  0.56  &     1.1 & --0.14 & 1.01\\
  UGC 1238 &  Sb       & 3  &  1.78 & 0.08& 0.12  & 0.75 &  2.05  &    3.78 &  0.03 & 0.77\\
  UGC 1248 &  Sa-b     & 6  &  3.16 & 0.09&$<$0.12  & 0.28 &  1.63  &    2.24 &  0.77 & 0.73\\
  UGC 1251 &  peculiar &    &  0.91 &$<$0.10& 0.18  & 0.03 &  0.55  &    0.59 &  0.83 & 0.62\\
  UGC 1302 &  SBb      & 3  &  2.45 & 0.11& 1.29  & 1.29 &  2.78  &    5.79 &   0.1 & 0.55\\
  UGC 1319 &  S?       &    &  0.89 & 0.12&$<$0.20  & 0.92 &  2.74  &    4.85 &  0.27 & 0.16\\
  UGC 1338 &  Sb       & 2  &  0.89 &$<$0.13&$<$0.13  & 0.29 &  0.85  &    1.52 &$>$0.79  & 0.21\\
  UGC 1344 &  SBa      & 5  &  1.62 &     &       &      &        &         &$>$0.78  & 0.21\\
  UGC 1347 &  Sc/SBc   & 1  &  1.26 & 0.12& 0.19  & 1.49 &  3.84  &    7.28 &--0.07  & 0.27\\
  UGC 1349 &  Sc       & 1  &  1.29 & 0.14& 0.21  & 1.44 &  3.26  &    6.61 & 0.38  & 0.05\\
  UGC 1358 &  S0-a     & 6  &  1.55 & 0.07&$<$0.04  & 0.09 &  0.31  &    0.51 &$>$0.79  & 0.09\\
  UGC 1376 &  SBb      & 4  &   1.7 &$<$0.10&$<$0.11  & 0.26 &   0.9  &    1.48 & 0.22  & 1.88\\
  UGC 1411 &  Sb       & 6  &  1.82 &$<$0.11&0.01   & 0.44 &  1.45  &    2.46 & --0.3  & 1.22\\
  UGC 1421 &  S        & 7  &  1.62 &$<$0.08&$<$0.09  &  0.3 &  0.98  &    1.67 &  0.48 & 1.86\\
  UGC 1422 &           &    &  1.17 &$<$0.09&$<$0.11  & 0.31 &  0.87  &     1.6 &  0.17 & 2.00\\
  UGC 1437 &  Sc       & 3  &  2.51 & 0.29& 0.38  & 3.36 &  11.4  &   19.04 & --0.15 & 0.58\\
  UGC 1456 &  Sa-b     & 3  &  1.26 & 0.09&$<$0.18  & 0.62 &   2.5  &     3.9 &  0.46 & 0.77\\
  UGC 1493 &  SB?a-b   & 6  &  1.82 & 0.16& 0.16  & 1.29 &  3.65  &    6.61 &  0.75 & 1.51\\
  UGC 1497 &  Sc       & 2  &  1.58 & 0.17& 0.29  & 2.02 &  5.85  &   10.49 & --0.09 & 2.64\\
  UGC 1520 &  peculiar &    &  0.63 & 0.14&$<$0.22  & 1.67 &  4.07  &    7.95 & --0.08 & 2.61\\
  UGC 1550 &  Sc       & 6  &  3.16 & 0.13& 0.22  & 1.45 &  5.06  &    8.34 &   0.1 & 1.74\\
  UGC 1581 &  S-Irr    &    &  1.66 &$<$0.11& 0.80  &  0.8 &   2.4  &    4.22 & --0.29 & 1.66\\
  UGC 1633 &  SBb-c    & 6  &  2.95 & 0.21& 0.25  & 1.91 &   6.2  &   10.55 &  0.21 & 2.36\\
  UGC 1655 &  peculiar &    &  2.88 & 0.70& 1.03  &10.89 & 22.83  &    48.3 &  0.25 & 2.64\\
  UGC 1672 &  S        & 6  &   1.1 & 0.37& 0.75  & 6.43 & 12.54  &   27.62 & --0.06 & 2.27\\
  UGC 1676 &  Sba/Sb   & 5  &  1.78 &$<$0.10&$<$0.12  & 0.86 &   2.6  &    4.57 &  0.06 & 2.26\\
  UGC 1721 &  SBb/SBc  & 1  &     2 &$<$0.11&$<$0.12  & 0.19 &  0.77  &     1.2 & --0.14 & 2.61\\
  UGC 1769 &  Sb/Sc    & 4  &     1 &0.08 &$<$0.14  & 0.68 &  2.33  &    3.86 & --0.31 & 2.98\\
  Z522-002 &           &    &  0.74 &$<$0.10&$<$0.07  &  0.3 &  0.71  &     1.4 & --0.21 & 1.02\\
  \hline
\end{tabular}                            
\label{Abell262-Properties}
\end{table}