  We show the preliminary results of the application of our "fireshell" model
to GRB060124. This source is very peculiar because it is the first event for
which both the prompt and the afterglow emission were observed simultaneously
by the three Swift instruments: BAT (15-350 keV), XRT (0.2-10 keV) and UVOT
(170-650 nm), due to the presence of a precursor ~ 570 s before the main burst.
We analyze GRB060124 within our "canonical" GRB scenario, identifying the
precursor with the P-GRB and the prompt emission with the afterglow peak
emission. In this way we reproduce correctly the energetics of both these two
components. We reproduce also the observed time delay between the precursor
(P-GRB) and the main burst. The effect of such a time delay in our model will
be discussed.
