All Figures

$\begin{figure} \par\includegraphics[height=0.3\textheight,clip]{0096fig1.eps}\end{figure}$ Figure 1: The contours with linear intervals are for the [O III]5007 Å emission from the giant lobe around P Cygni. These are overlain on a negative grey-scale presentation of the H $\alpha$ and [N II] 6548 & 6584 Å emission. Areas affected by the scattered light from the central star are blanked out. The black circle around P Cygni depicts the extent of the outer shell (OS) and the MES slit positions A and B where the spectra in Fig. 2 were obtained are also shown. Coordinates are J2000.
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In the text

$\begin{figure} \par\includegraphics[height=0.49\textheight,clip]{0096fig2.eps}\end{figure}$ Figure 2: Grey-scale representations of the position-velocity arrays of [N II]6584 Å line profiles along the slit positions A and B (see Fig. 1) are shown. The line profiles along slit length A over the northerly ridge (marked GL north) and the newly discovered southerly ridge (marked GL south) can be appreciated. The spectral features from the outer shell (marked OS) are distinguished from those of the westerly giant lobe (marked GL west) along slit length B. The systemic heliocentric radial velocity (-26 km s^-1) of P Cygni is arrowed. This was given by the central velocity of the OS assuming spherical expansion.
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In the text

$\begin{figure} \par\includegraphics[height=0.82\textheight,clip]{0096fig3.eps}\end{figure}$ Figure 3: a) The filaments that could possibly be giant lobes projecting from the LBV star R 143 in the LMC can be seen in this H $\alpha$ plus [N II] 6548 & 6584 Å image and are indicated by GL? b) These faint northern filaments connect with the bright ridges near to this star. Coordinates are J2000.
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In the text

$\begin{figure} \par\includegraphics[height=0.82\textheight,clip]{0096fig3.eps}\end{figure}$	Figure 3: a) The filaments that could possibly be giant lobes projecting from the LBV star R 143 in the LMC can be seen in this H $\alpha$ plus [N II] 6548 & 6584 Å image and are indicated by GL? b) These faint northern filaments connect with the bright ridges near to this star. Coordinates are J2000.
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