Fig. 12.
Download original image
Specific ccSN rate per unit stellar mass as a function of host galaxy stellar mass. The blue and orange markers indicate the rates for SNe II and SESNe, respectively. The estimated stellar masses of the Small Magellanic Cloud (Montes et al. 2024), Large Magellanic Cloud (van der Marel et al. 2002), M33 (Corbelli et al. 2014), and M31 (Sick et al. 2015) are shown at the top of the panel. The top panel shows the distribution of host galaxy stellar mass.
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.