![\begin{figure}
\par\includegraphics[width=8.8cm,clip]{8783fig1.eps}
\end{figure}](/articles/aa/full/2008/32/aa8783-07/img37.gif) |
Figure 1: Schematic two jets scenario for GRB 060206. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[angle=0,width=9cm,clip]{8783fig2.eps}
\end{figure}](/articles/aa/full/2008/32/aa8783-07/img173.gif) |
Figure 2:
R-band light curve of
GRB 060206. ``FE''
and ``RE'' represent the forward shock emission and the reverse
shock emission, respectively. The dotted line
represents the contribution from Jet A. The thick, dashed
line and the thin, dashed line correspond to the emissions from the
forward shock and the reverse shock of Jet B,
respectively. The dash-dotted lines represent the emission
from Jet B taking into account the zero-time effect. The
thick, solid line includes the contribution from both Jet A and Jet B. R-band data are taken from
Monfardini et al. (2006), Stanek et al. (2007) and
et al. (2006). |
| Open with DEXTER | |
In the text