Fig. 10
Left: the completeness-corrected LFs in the MKs for the M-giants and C stars. The inner small panel in the lower panel indicates the logarithmic LF of M-giant of NGC 205. The LFs with solid lines show the M-giants and C stars detected in the WIRCam field of NGC 205. Right: the completeness-corrected bolometric LFs for the M-giants and C stars.
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.