Fig. 8.
Download original image
Abundances of different galaxy properties in the five groups of MaNGA galaxies classified based on the ex situ stellar mass fraction gradient in their inner parts. From top to bottom, the different rows illustrate how each group differs in morphology, star formation activity, rotation, host dark matter halo mass, and environment.
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.