![\begin{figure}
\par\includegraphics[height=3.2cm,width=6.6cm,clip]{7391Fig1.eps}\end{figure}](/articles/aa/full/2007/20/aa7391-07/img40.gif){kind=small} |
Figure 1: The density profile of the CBM in our model. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[height=3.45cm,width=7.2cm,clip]{7391Fig2.eps}\end{figure}](/articles/aa/full/2007/20/aa7391-07/img47.gif){kind=small} |
Figure 2:
The variation in the maximum
Lorentz factor. We also plot the Lorentz factor at the forward
shock. The variation is presented a function of the distance and in
the lab-frame time. Note the change from log to linear scale at
 . |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[height=3.41cm,width=7.2cm,clip]{7391Fig3.eps}\end{figure}](/articles/aa/full/2007/20/aa7391-07/img48.gif){kind=small} |
Figure 3: The variation in the (logarithm of) maximum pressure as a function of the distance and the comoving frame time. |
| Open with DEXTER | |
In the text
![\begin{figure}
\includegraphics[height=2.3cm,width=6.3cm,clip]{7391Fig4a.eps}\pa...
...s}\par\includegraphics[height=2.3cm,width=6.3cm,clip]{7391Fig4f.eps}\end{figure}](/articles/aa/full/2007/20/aa7391-07/img64.gif) |
Figure 4:
All zones present when the relativistic shell interacts
with the CBM. The shell profile is shown at three different times: from top
down: at time
after the rapid thermal acceleration;
at time
 ,
prior to the encounter with the wind
termination shock at time
 .
The first three
frames show the logarithm of density in the lab-frame, the last three
show kinetic energy. |
| Open with DEXTER | |
In the text