Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=5.7cm,clip]{aa5289f1.ps}\end{figure}$ Figure 1: Distribution of velocity-integrated H₃O⁺ 364 GHz emission toward Sgr B2, observed with the APEX telescope. Filled dots indicate detections; open dots denote upper limits. The greyscale runs from 1.9 to 35.5 in steps of 3.7 K km s^-1.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.7cm,clip]{aa5289f1.ps}\end{figure}$	Figure 1: Distribution of velocity-integrated H₃O⁺ 364 GHz emission toward Sgr B2, observed with the APEX telescope. Filled dots indicate detections; open dots denote upper limits. The greyscale runs from 1.9 to 35.5 in steps of 3.7 K km s^-1.
Open with DEXTER

$\begin{figure} \par\hspace*{2mm}\includegraphics[angle=-90,width=7.65cm,clip]{aa5289f2.ps} \includegraphics[angle=-90,width=7.5cm,clip]{aa5289f3.ps}\end{figure}$	Figure 2: Spectra of the H₃O⁺ 364 GHz line ( top) and 307 GHz line ( bottom) toward the Sgr B2 (M) and Sgr B2 (OH) positions.
Open with DEXTER