Free Access

Fig. 26.

image

Same as Fig. 6, but now comparing the photospheric properties for models r0e2 (smooth ejecta) and r0e2cl (same as model r0e2 but the ejecta is clumped, with a 10% volume filling factor). The clumped model is initially similar to the smooth counterpart, but as time progresses after bolometric maximum (which occurs in both at about 30 d), the clumped ejecta cools and recombines faster, entering the nebular phase 150 d after explosion, which is 30 d earlier than in model r0e2.

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.