Fig. 10
Download original image
AMR for the NGC 1023 GC system based on DynBaS 3 (blue circles) compared to 3 E-MOSAIC simulations: MW014, MW016, and MW023 from Kruijssen et al. (2019a) (grey contours) that have comparable halo masses to NGC 1023. We observe a (likely) broad AMR of NGC 1023 GC system, where the objects have a broad metallicity distribution and are mainly old.
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.