Figure 2: The fit of the theory to the photometric observations 970422-4O3-d. The time is measured from Apr. 22, 1997 |
Figure 7: The fit of the theory to the photometric observations 970718-3O2-a (dots) and 970718-3O2-g (circles) |
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) |
Figure 11: The fit of the theory to the photometric observations 970725-3E2-a (circles), 970725-3E2-k (dots) and 970725-3E2-g (squares) |
Figure 12: The fit of the theory to the photometric observations 970725-3O2-k (dots, dashed line) and 970725-3O2-t (circles) |
Figure 13: The fit of the theory to the photometric observations 970731-4E3-e. The time is measured from July 31, 1997 |
Figure 14: The fit of the theory to the photometric observations 970801-4E2-g (circles, dashed line) and 970801-4E2-l (dots) |
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 Aug. 2, 1997 |
Figure 25: The fit of the theory to the photometric observations 970918-1E3-e (dots, dashed line) and 970918-1E3-t (circles) |
Figure 29: The fit of the theory to the photometric observations 971109-4O2-t (dots, dashed line), 971109-4O2-w (circles) |
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