Open Access

Fig. 6.

image

Download original image

Relative mass fraction of disk structures of tiny-halo (blue) and halo-subdominated (red) galaxies, measured using morphological fdisk, morph and kinematic fdisk, kinem methods. The morphologically defined disks are generally 10% larger than those defined in the kinematical method from Du et al. (2019, 2020). The envelopes of shaded regions represent the 16th and 84th percentiles and the solid profile is the median value.

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.