Fig. 10.
Download original image
Comparison between the bolometric light curve of SN 2024bch and ‘Model A’ from Dessart et al. (2016), which was built to explain the luminosity evolution of SN 1998S. The model fails to reproduce both the fast rise and the overall luminosity of SN 2024bch, which suggests that ejecta-CSM interaction does not play a role in powering its light curve.
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.