Characterising the orbit and circumstellar environment of the high-mass binary MWC 166 A

Open Access

Fig. 9.

Hertzsprung-Russell diagram showing PARSEC 1.2S isochrone tracks for each age. Superimposed are the interpolated L, T_eff values for the primary star (large circles) and secondary star (triangles), for all ages. The black cross shows the location of the primary’s parameters as determined by Fairlamb et al. (2015).

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.