Fig. 5.

Download original image
Energy-angular momentum relation for the SNd-like region for all (top two rows), in situ (third row), and accreted (bottom row) populations. The first and second rows are coloured by the stellar number density and the mean stellar metallicity, respectively. In the bottom two rows, the colour corresponds to mean metallicity. The coloured boxes in the top row show the selection of retrograde (red), non-rotating (blue), and prograde (yellow) stellar populations that are featured in Fig. 6. The energy is normalised to the mean energy of the corresponding sample for a given galaxy, marked at the bottom of each top panel and in units of 106 kpc × km2 s−2.
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.