Masses and radii of M-dwarfs in five EBLM systems. The 5 Gyr isochrone for solar metallicity from Baraffe et al. (2015) is plotted (black-solid) along with the 5 Gyr isochrone for [M/H] = −0.5 (Baraffe et al. 1998; black-dashed). We plot low-mass M-dwarfs with masses and radii known to better than 10% (from Table 4 of Chaturvedi et al. 2018, and references therein). For J2308−46 and J0218−31 we plot both solutions and label accordingly. We also plot TRAPPIST-1 (Delrez et al. 2018), Proxima Centauri (Anglada-Escudé et al. 2016) and J0555−57 (von Boetticher et al. 2017).
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.