Free Access

Fig. 21.

image

Bolometric light curves for models r0e2 and r0e2ba, which differ only in magnetar field strength. The thin solid and dashed lines correspond to the instantaneous magnetar power absorbed by each ejecta. The contribution from 0.13 M of 56Ni is in part responsible for the offset after 100 d. This offset is small in the model r0e2ba due to the much greater magnetar power at late times.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.