![\begin{figure}
\par\includegraphics[width=15.7cm,clip]{0212fig4.eps}\par
\end{figure}](/articles/aa/full/2004/11/aa0212/Timg126.gif) |
Figure 4:
The shaded areas indicate the most likely values of
magnetic fields just behind the shock front
and
the maximum energy of shock-accelerated electrons
.
The left panel is for the age-limited case, while
the right gives the energy loss-limited model.
These areas are formed by the two solid lines for
a roll-off energy of
-3.3)
Hz,
and the two dashed lines from
the observed width of nonthermal X-rays;
in the age-limited case,
a gyro-radius of accelerated electrons in the downstream
should be
-20
pc,
while in the energy loss-limited case,
cooling time of accelerated electrons
should be
-5.4
yrs. |