Fig. 10
Download original image
Radio images show a bilateral G309.2-00.6 (top panel, Ferrand & Safi-Harb 2012) and the Cygnus Loop (bottom panel, Uyaniker et al. 2004) CCSNRs. This study conjectures that bilateral remnants from massive stars are less common than those of Cygnus Loops but also that these shapes constitute a time-sequence of morphological evolution affecting the remnants of the most common runaway red supergiant progenitors.
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.