$\begin{figure} \par\includegraphics[width=15.5cm,clip]{odin8.f1} \end{figure}$ Figure 1: The 557-GHz H₂¹⁶O line profiles observed towards a) the Sgr $\rm {A}^{\star }$ Circumnuclear Disk, the b) +20 and c) +50 km s^-1 clouds, and d) the 548-GHz H₂¹⁸O isotope line profile observed towards the Sgr $\rm {A}^{\star }$ Circumnuclear Disk.
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In the text

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{odin8.f2} \end{figure}$ Figure 2: The SEST C¹⁸O (1-0) survey Odin-beam convolved profiles towards a) the Sgr $\rm {A}^{\star }$ Circumnuclear Disk, the b) +20 and c) +50 km s^-1 clouds.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{odin8.f3} \end{figure}$ Figure 3: Gaussian analysis performed on the 557-GHz H₂¹⁶O line profile observed towards the Sgr $\rm {A}^{\star }$ Circumnuclear Disk.
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In the text

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{odin8.f1} \end{figure}$	Figure 1: The 557-GHz H₂¹⁶O line profiles observed towards a) the Sgr $\rm {A}^{\star }$ Circumnuclear Disk, the b) +20 and c) +50 km s^-1 clouds, and d) the 548-GHz H₂¹⁸O isotope line profile observed towards the Sgr $\rm {A}^{\star }$ Circumnuclear Disk.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{odin8.f2} \end{figure}$	Figure 2: The SEST C¹⁸O (1-0) survey Odin-beam convolved profiles towards a) the Sgr $\rm {A}^{\star }$ Circumnuclear Disk, the b) +20 and c) +50 km s^-1 clouds.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{odin8.f3} \end{figure}$	Figure 3: Gaussian analysis performed on the 557-GHz H₂¹⁶O line profile observed towards the Sgr $\rm {A}^{\star }$ Circumnuclear Disk.
Open with DEXTER