Numerical Experiments for Nuclear Flashes toward Superbursts in an Accreting Neutron Star
Figure 6
Light curves at s (a) and that from s (b). corresponds to the same epoch as shown by the mark in Figure 9. The interval between s is named the “log interval 1.” Marks of 1–5 and 6 are successive numbers and a sign of each burst before and after “long interval 1,” respectively.
