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Figures 1-31


 \begin{figure}\psfig{file=fig1.eps,width=10cm}
\end{figure} Figure 1: The fit of the theory to the photometric observations 970413-1O2-d


 \begin{figure}\psfig{file=fig2.eps,width=10cm}
\end{figure} Figure 2: The fit of the theory to the photometric observations 970422-4O3-d. The time is measured from $0^ {\rm h}$ Apr. 22, 1997


 \begin{figure}\psfig{file=fig3.eps,width=10cm}
\end{figure} Figure 3: The fit of the theory to the photometric observations 970622-1E2-a


 \begin{figure}\psfig{file=fig4.eps,width=10cm}
\end{figure} Figure 4: The fit of the theory to the photometric observations 970706-3E4-v


 \begin{figure}\psfig{file=fig5.eps,width=10cm}
\end{figure} Figure 5: The fit of the theory to the photometric observations 970715-1O3-a


 \begin{figure}\par\psfig{file=fig6.eps,width=10cm}
\end{figure} Figure 6: The fit of the theory to the photometric observations 970718-3E2-a


 \begin{figure}\psfig{file=fig7.eps,width=10cm}
\end{figure} Figure 7: The fit of the theory to the photometric observations 970718-3O2-a (dots) and 970718-3O2-g (circles)


 \begin{figure}\psfig{file=fig8.eps,width=10cm}
\end{figure} Figure 8: The fit of the theory to the photometric observations 970719-3O1-a


 \begin{figure}\par\psfig{file=fig9.eps,width=10cm}
\end{figure} Figure 9: The fit of the theory to the photometric observations 970724-1E4-a


 \begin{figure}\par\psfig{file=fig10.eps,width=10cm}
\end{figure} Figure 10: The fit of the theory to the photometric observations 970725-1E4-a (squares), 970725-1E4-g (dots, dashed line) and 970725-1E4-t (circles)


 \begin{figure}\par\psfig{file=fig11.eps,width=10cm}
\end{figure} Figure 11: The fit of the theory to the photometric observations 970725-3E2-a (circles), 970725-3E2-k (dots) and 970725-3E2-g (squares)


 \begin{figure}\par\psfig{file=fig12.eps,width=10cm}
\end{figure} Figure 12: The fit of the theory to the photometric observations 970725-3O2-k (dots, dashed line) and 970725-3O2-t (circles)


 \begin{figure}\par\psfig{file=fig13.eps,width=10cm}
\end{figure} Figure 13: The fit of the theory to the photometric observations 970731-4E3-e. The time is measured from $0^ {\rm h}$ July 31, 1997


 \begin{figure}\par\psfig{file=fig14.eps,width=10cm}
\end{figure} Figure 14: The fit of the theory to the photometric observations 970801-4E2-g (circles, dashed line) and 970801-4E2-l (dots)


 \begin{figure}\par\psfig{file=fig15.eps,width=10cm}
\end{figure} Figure 15: The fit of the theory to the photometric observations 970801-4E3-k


 \begin{figure}\par\psfig{file=fig16.eps,width=10cm}
\end{figure} Figure 16: The fit of the theory to the photometric observations 970803-4E1-k (dots), 970803-4E1-l (squares) and 970803-4E1-t (circles). The time is measured from $0^ {\rm h}$ Aug. 2, 1997


 \begin{figure}\psfig{file=fig17.eps,width=10cm}
\end{figure} Figure 17: The fit of the theory to the photometric observations 970830-3E2-a


 \begin{figure}\par\psfig{file=fig18.eps,width=10cm}
\end{figure} Figure 18: The fit of the theory to the photometric observations 970830-3O2-a


 \begin{figure}\par\psfig{file=fig19.eps,width=10cm}
\end{figure} Figure 19: The fit of the theory to the photometric observations 970903-1E3-a


 \begin{figure}\par\psfig{file=fig20.eps,width=10cm}
\end{figure} Figure 20: The fit of the theory to the photometric observations 970906-3O2-g


 \begin{figure}\par\psfig{file=fig21.eps,width=10cm}
\end{figure} Figure 21: The fit of the theory to the photometric observations 970910-1O3-a


 \begin{figure}\par\psfig{file=fig22.eps,width=10cm}
\end{figure} Figure 22: The fit of the theory to the photometric observations 970914-3E1-e


 \begin{figure}\par\psfig{file=fig23.eps,width=10cm}
\end{figure} Figure 23: The fit of the theory to the photometric observations 970915-3E2-a


 \begin{figure}\par\psfig{file=fig24.eps,width=10cm}
\end{figure} Figure 24: The fit of the theory to the photometric observations 970918-1O3-g


 \begin{figure}\par\psfig{file=fig25.eps,width=10cm}
\end{figure} Figure 25: The fit of the theory to the photometric observations 970918-1E3-e (dots, dashed line) and 970918-1E3-t (circles)


 \begin{figure}\par\psfig{file=fig26.eps,width=10cm}
\end{figure} Figure 26: The fit of the theory to the photometric observations 970921-3E1-l


 \begin{figure}\psfig{file=fig27.eps,width=10cm}
\end{figure} Figure 27: The fit of the theory to the photometric observations 970922-3E2-g


 \begin{figure}\par\psfig{file=fig28.eps,width=10cm}
\end{figure} Figure 28: The fit of the theory to the photometric observations 971007-4O1-t


 \begin{figure}\par\psfig{file=fig29.eps,width=10cm}
\end{figure} Figure 29: The fit of the theory to the photometric observations 971109-4O2-t (dots, dashed line), 971109-4O2-w (circles)


 \begin{figure}\psfig{file=fig30.eps,width=10cm}
\end{figure} Figure 30: The fit of the theory to the photometric observations 971110-3E1-t


 \begin{figure}\psfig{file=fig31.eps,width=10cm}
\end{figure} Figure 31: The fit of the theory to the photometric observations 971118-3O1-g


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