Fig. 1
Download original image
Schematic (not to scale) of a SNR evolving within a bipolar CSM created by a stellar eruption, subsequent to the ejection of the stellar wind. Panel a shows the expansion of the SN ejecta and the forward shock at early times after the explosion. Panel b presents the time when the SN begins to interact with the densest medium left by the eruption.
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.