Comparing the spatial and kinematic distribution of gas and young stars around the shell-like structure in the CMa OB1 association

Free Access

Fig. 2

DSS2-Red image of the Sh 2-296 nebula. The ellipse marks the proposed shape of the CMa shell and the contours in each panel trace: (a) the ¹³CO emission (courtesy of the Osaka group, see Onishi et al. 2013); (b) extinction (A_V) from the 2MASS maps of Dobashi et al. (2011). The figure is adapted from Fernandes et al. (2019).

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.