Free Access

Fig. 7.

image

Download original image

Ratio of the distances derived in this work (DI, Table 4), with the average distances from Baumgardt & Vasiliev (2021, BV21, left panel) and the distances derived from parallaxes from Vasiliev & Baumgardt (2021, VB21, right panel). The vertical error bars correspond to the derived uncertainties, divided by DBV21 or DVB21. The distances from Vasiliev & Baumgardt (2021) are discrepant with ours only for the three closest GCs (10% for NGC 6626, and 20% for NGC 6266 and NGC 6717).

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.