Astronomy & Astrophysics

All Figures

$\begin{figure} \par\resizebox{8.1cm}{!}{\includegraphics[clip]{aa0314f1.ps}} \end{figure}$ Figure 1: Gray-scale representation with overlaid isocontours of the ISOPHOT ${\rm 90~\mu m}$ map of the region north of NGC 5128. The large dark blob at the bottom is the FIR emission of the central dusty disk region of NGC 5128 itself. Only a few very low level structures near the edges of the mapped region are apparent. Map pixel size is $35\hbox {$^{\prime \prime }$ }$ .
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In the text

$\begin{figure} \par\resizebox{8.3cm}{!}{\includegraphics[clip]{aa0314f2.ps}} \end{figure}$ Figure 2: Gray-scale representation with overlaid isocontours of the ISOPHOT ${\rm 150~\mu m}$ map. In addition to the strong FIR emission of the central region of NGC 5128 near the lower edge, a resolved emission region ${\approx }15\hbox {$^\prime $ }$ northeast of NGC 5128 (marked with a bar) can clearly be seen. Map pixel size is $40\hbox {$^{\prime \prime }$ }$ .
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In the text

$\begin{figure} \par\resizebox{8.2cm}{!}{\includegraphics[clip]{aa0314f3.ps}} \end{figure}$ Figure 3: Same as Fig. 2, but for the ${\rm 200~\mu m}$ band.
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In the text

$\begin{figure} \par\resizebox{8.3cm}{!}{\includegraphics[clip]{aa0314f4.eps}} \end{figure}$ Figure 4: Gray-scale representation of the ISOPHOT ${\rm 200~\mu m}$ map with overlaid isocontours of the DSS-2 B-band image. The outlying FIR emission region is indicated by the white ellipse.
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In the text

$\begin{figure} \par\resizebox{7.9cm}{!}{\includegraphics[clip]{aa0314f5.ps}} \end{figure}$ Figure 5: FIR spectrum of the off-center source at the position of the HI/CO detection in NGC 5128. 30% error bars are indicated for the ISOPHOT detections at ${\rm 150~\mu m}$ and ${\rm 200~\mu m}$ . The dashed curve shows a modified blackbody spectrum with temperature $T{\rm _{Dust} = 13~K}$ and emissivity ${\rm\beta = 2}$ .
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In the text

$\begin{figure} \par\resizebox{8.1cm}{!}{\includegraphics[clip]{aa0314f1.ps}} \end{figure}$	Figure 1: Gray-scale representation with overlaid isocontours of the ISOPHOT ${\rm 90~\mu m}$ map of the region north of NGC 5128. The large dark blob at the bottom is the FIR emission of the central dusty disk region of NGC 5128 itself. Only a few very low level structures near the edges of the mapped region are apparent. Map pixel size is $35\hbox {$^{\prime \prime }$ }$ .
Open with DEXTER

$\begin{figure} \par\resizebox{8.3cm}{!}{\includegraphics[clip]{aa0314f2.ps}} \end{figure}$	Figure 2: Gray-scale representation with overlaid isocontours of the ISOPHOT ${\rm 150~\mu m}$ map. In addition to the strong FIR emission of the central region of NGC 5128 near the lower edge, a resolved emission region ${\approx }15\hbox {$^\prime $ }$ northeast of NGC 5128 (marked with a bar) can clearly be seen. Map pixel size is $40\hbox {$^{\prime \prime }$ }$ .
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$\begin{figure} \par\resizebox{8.2cm}{!}{\includegraphics[clip]{aa0314f3.ps}} \end{figure}$	Figure 3: Same as Fig. 2, but for the ${\rm 200~\mu m}$ band.
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$\begin{figure} \par\resizebox{8.3cm}{!}{\includegraphics[clip]{aa0314f4.eps}} \end{figure}$	Figure 4: Gray-scale representation of the ISOPHOT ${\rm 200~\mu m}$ map with overlaid isocontours of the DSS-2 B-band image. The outlying FIR emission region is indicated by the white ellipse.
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$\begin{figure} \par\resizebox{7.9cm}{!}{\includegraphics[clip]{aa0314f5.ps}} \end{figure}$	Figure 5: FIR spectrum of the off-center source at the position of the HI/CO detection in NGC 5128. 30% error bars are indicated for the ISOPHOT detections at ${\rm 150~\mu m}$ and ${\rm 200~\mu m}$ . The dashed curve shows a modified blackbody spectrum with temperature $T{\rm _{Dust} = 13~K}$ and emissivity ${\rm\beta = 2}$ .
Open with DEXTER