![\begin{figure}
\par\includegraphics[width=8cm,clip]{Gk191_f1.ps}\end{figure}](/articles/aa/full/2005/14/aagk191/img6.gif) |
Figure 1: Lightcurve of the source ( upper panel) and the background ( lower panel) during March 4, 2003 observation of IGR/AX J16320-4752 with XMM-Newton. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.6cm,clip]{Gk191_f2.ps}\end{figure}](/articles/aa/full/2005/14/aagk191/img8.gif) |
Figure 2:
distribution obtained while folding the source and the
background lightcurves during March 4, 2003 observation of IGR/AX J16320-4752 with XMM-Newton. It is seen that the background lightcurves does not demonstrate a coherent signal with the period
of  1300 s. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.25cm,clip]{Gk191_f3.ps}\end{figure}](/articles/aa/full/2005/14/aagk191/img9.gif) |
Figure 3:
Lightcurve of IGR/AX J16320-4752 obtained by ASCA/GIS ( upper panel)
and distribution obtained while folding this lightcurve for
various trial periods ( lower panel). |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.25cm,clip]{Gk191_f4.ps}\end{figure}](/articles/aa/full/2005/14/aagk191/img17.gif){kind=small} |
Figure 4: Pulse profile of IGR/AX J16320-4752 obtained in the 1-10 keV energy band by folding of the XMM-Newton lightcurve with the period of 1309 s. |
| Open with DEXTER | |
In the text