Fig. 5
Colour magnitude plots for (candidate) LBVs within M 33, following the ammended classification scheme of Ma07. Stars associated with hot dust are identified in Sect. 4.2. Note that Massey et al. (1996) associate the brightest object, J013350.92+303936.9 (=UIT218), with the galactic nucleus – an apparently composite source with an F Ia spectral type rather the hot LBV classification given in Ma07 – while J013242.26-301214.1 lacks an (R − I) indice.
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.