Highlight
Free Access

Fig. 4

thumbnail

All 58 microlensed dwarf stars plotted on the α-enhanced isochrones from Demarque et al. (2004). The metallicity of the stars in each panel is within  ±0.05 dex of the isochrone metallicity. In each plot the solid lines represent isochrones with ages of 0.1, 5, 10, 15, and 20 Gyr. Dotted lines are isochrones in steps of 1 Gyr. Error bars represent the uncertainties in Teff and log g as given in Table 4. Note that the age determinations reported in Table 5 are based on probability distribution functions as described in Bensby et al. (2011).

This figure is made of several images, please see below:

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.