NGC 6752 AGB stars revisited - I. Improved AGB temperatures remove apparent overionisation of Fe i

Free Access

Fig. 10

Open with DEXTER Download original image

Our final stellar parameters for the NGC 6752 AGB and RGB stars. All are “photometric” – based on the IRFM temperatures calculated for this study, except for 2 AGB stars (see Fig. 9).

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.