Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{1820Fig1.eps} \end{figure}$ Figure 1: Coronagraphic image of NGC 1068. A log-scale representation is used for more clarity. North is up and east is left. Top: the whole field: $11.7\hbox {$^{\prime \prime }$ }\times 11.7\hbox {$^{\prime \prime }$ }$ , bottom: zoom on filamentary structures south west. The color distribution have been chosen to ensure a good contrast in large scale structures.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1820Fig2.eps} \end{figure}$ Figure 2: Top: NGC 1068, Ks band with NACO, without mask. Bottom: reference subtracted coronographic image of NGC 1068 in a log-scale representation. The color distribution has been chosen to ensure a good contrast for structures close to the nucleus.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1820Fig1.eps} \end{figure}$	Figure 1: Coronagraphic image of NGC 1068. A log-scale representation is used for more clarity. North is up and east is left. Top: the whole field: $11.7\hbox {$^{\prime \prime }$ }\times 11.7\hbox {$^{\prime \prime }$ }$ , bottom: zoom on filamentary structures south west. The color distribution have been chosen to ensure a good contrast in large scale structures.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{1820Fig2.eps} \end{figure}$	Figure 2: Top: NGC 1068, Ks band with NACO, without mask. Bottom: reference subtracted coronographic image of NGC 1068 in a log-scale representation. The color distribution has been chosen to ensure a good contrast for structures close to the nucleus.
Open with DEXTER