Temperature–luminosity plots of the nongiant stars observed in Lupus 1, 3, and 4. Superimposed are selected evolutionary tracks of Baraffe et al. (1998) for stars above the substellar limit, merged with those of Chabrier et al. (2000) for brown dwarfs with dusty atmospheres. Objects with estimated log g ≃ 3.5 are marked as asterisks; those with log g ≃ 4.0, with crosses; and those with log g ≃ 4.5−5.0, with three-pointed 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.