Fig. 30.
Download original image
Photospheric velocity evolution of SN 2018ibb (probed with Fe II) and the predicted evolution from different PISN models. The synthetic velocities of the P250Ni25|34 and He130 models are very similar to the observed velocities and velocity evolution. These are also the models that match the observed bolometric light curve well, in particular the He130 model.
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.