\begin{table}%t1
\par
   \caption {\label{tab:morph}PNe containing close binary central stars whose nebular morphologies are assessed in this work. 
   }
%\centerline
 {      \begin{tabular}{llrrlrlllll}
      \hline\hline
PN G & Name  & Period  & Diameter & Eclipsing   &$i$ (lit.)&Model/$i$& Morphology & Traits &         IRAC & Ref.\\
&       & (days)     &     (arcsec)       & &(deg)&&     &      &   1~~ 2~ 3~ 4 &        \\
\hline
005.0$+$03.0 & Pe 1-9          &0.14& 12 $\times$ 14& Y  &$\sim$90&--& MS &  L                        & N U N U &b\\
355.3$-$03.2 & PPA 1747$-$3435 &0.22& 12 & N  &--&--&  Irr & --                      & U U U U&a \\
355.7$-$03.0 & H 1-33          &1.13& 5 $\times$ 12 & N  &--&A/45& CB & G                        & U Y U \textbf{Y}  &a \\
354.5$-$03.9 & Sab 41          &0.30& 95 $\times$ 194 & N  &--&A/40& LB & L, J, R                        & U U U U        & b \\
000.6$-$01.3 & Bl 3-15         &0.27& 4 $\times$ 11 & N &--& A&  LB & G, J              & Y Y \textbf{Y} \textbf{Y} & a \\
359.1$-$02.3 & M 3-16          &0.57& 9 $\times$ 13& Y  &$\sim$90&--& Irr &  L, J                       & Y \textbf{Y} Y \textbf{Y} & b\\
357.6$-$03.3 & H 2-29          &0.24& 11 $\times$ 14 & Y  &$\sim$90&A/90& CB &  L, R                        & U U U U      &b \\
000.2$-$01.9 & M~2-19          &0.67& 7 $\times$ 19 & N  &--&A/45& CB &  G, R                        & Y Y Y \textbf{Y}& b \\
358.7$-$03.0 & K 6-34          &0.20& 14& N  &--&--&  MS/LB & G, L, J?, R              & N N N Y &b \\
357.0$-$04.4 & PHR~1756$-$3342 &0.26& 22 & N  &--&B/30&  PB & --                        & U U U U &b \\
001.8$-$02.0 & PHR~1757$-$2824 &0.80& 4 $\times$ 18 & Y  &$\sim$90&A/90&  CB & --                        & N N N N  &b \\
001.2$-$02.6 & PHR~1759$-$2915 &1.10& 25 $\times$ 30 & Y  &$\sim$90&A/90&  CB & --                        & N N N N &b \\
000.5$-$03.1a& MPA~1759$-$3007 &0.50& 17 $\times$ 42 & N  &--&A/55& LB & --                        & U N U N  &b \\
001.9$-$02.5 & PPA 1759$-$2834 &0.31& 17 $\times$ 35 & N  &--&B/45&  LB & I                        & N N N N &b \\
357.1$-$05.3 & BMP 1800$-$3408 &0.14& 30 $\times$ 55 & Y  &$\sim$90&--&  Irr & I                       & U U U U &b \\
000.9$-$03.3 & PHR~1801$-$2947 &0.32& 34 & N  &--&B/30&  PB & --                       & N N N N  &b \\
001.8$-$03.7 & PHR~1804$-$2913 &6.66& 3.5, 8 & N  &--&--&  MS & I                        & U N N N       &b \\
004.0$-$02.6 & PHR~1804$-$2645 &0.62&   24 $\times$ 45& Y &$\sim$90&A/90& CB &  G                        & N N N Y       &b \\
\hline                                                                                 
144.8$+$65.8 & BE UMa          &2.29& 180 & Y  &84 &A/85& LB &  --                        &  U U U U  &j, n\\
055.4$+$16.0 & A 46            &0.47& 53 $\times$ 70& Y  &80 &A/80& LB &  I                      & U U U U  &b, c, g\\
053.8$-$03.0 & A 63            &0.46& 42 $\times$ 290& Y  &88 &A/90& CB & J                        & U U U U  &g \\
136.3$+$05.5 & HFG 1           &0.58& 540& N  &28 &--&  Irr &I, L                      &  U U U U &f\\
253.5$+$10.7 & K 1-2           &0.68& 50 $\times$ 130 & N  &$\sim$45 &A/45&  LB & L, J                       & U U U U &b, i, m\\
283.9$+$09.7 & DS 1            &0.36& 290 $\times$ 335& N  &62&--& PB & I, L                      &  U U U U &b \\
329.0$+$01.9 & Sp 1            &2.91& 120 & N  &--&A/5& LB &  G, R               &  Y \textbf{Y} Y \textbf{Y} &c \\
349.3$-$01.1 & NGC 6337        &0.17& 60 $\times$100& N  &9&A/10& LB &  G, L, J, R                        &  Y \textbf{Y} Y \textbf{Y}    & l \\
005.1$-$08.9 & Hf 2-2          &0.40& 25 & N  &--&--&  MS & L, R                       &  U U U U &b, d \\
017.3$-$21.9 & A 65            &1.00& 220 $\times$ 240& N  &--&A/10& LB & J                      &  U U U U &e, h\\
009.6$+$10.5 & A 41            &0.23& 15 $\times$ 22& N  &66 & A/70 & CB &  R                        & U U U U &b, g \\
335.2$-$03.6 & HaTr 4          &1.74& 24 $\times$ 30 & N  &--&B/45 & PB &  --                        &  U U U U &c \\
215.6$+$03.6 & NGC 2346       &15.99& 58 $\times$ 172 & N  &50&A/50& CB & G, R                        &  Y Y \textbf{Y} \textbf{Y} & c \\
135.9$+$55.9 & SBS 1150$+$599A &0.16& 4 & N  &--&--& Irr & L?                       &  \textbf{Y} \textbf{Y} Y Y & k\\
341.6$+$13.7 & NGC 6026        &0.53& 60& N  &82&--& Irr & --                     &  U U U U &d \\
      \hline
   \end{tabular}
}
\par
\smallskip
      {\it Morphologies:} CB: Canonical bipolar; LB: Likely bipolar; PB: Possible bipolar; MS: Multiple shells; Irr: Irregular. \\
      {\it Morphological Traits:} G: Gatley's rule satisfied; I: ISM interaction; L: Low-ionisation knots or filaments; J: Jets; R: Equatorial ring.\\
      {\it IRAC:} U: Unavailable; Y: Nebular detection; N: Nebular non-detection.\\ 
      {\it References:} (a) Paper I, (b) this work, (c) Bond \& Livio (\cite{Bond90}), (d) Schwarz et~al. (\cite{Schwarz92}), (e) Walsh \& Walton (\cite{Walsh96}),  (f) 
      Heckathorn et~al.  (\cite{Heckathorn82}), (g) Pollacco \& Bell (\cite{Pollacco97}), (h) 
      Hua et~al.  (\cite{Hua98}), (i) Corradi et~al. (\cite{Corradi99}), (j) Bond (\cite{Bond00}),  (k) De Marco (\cite{DeMarco09}), (l) Corradi et~al. (\cite{Corradi00}), (m) 
      Exter et~al. (\cite{Exter03}), (n) Liebert et~al. (\cite{Liebert95}).  
\end{table}