Fig. 3
Measurements of orbital obliquity for the known transiting extrasolar planetary systems and brown dwarf companions in front of the effective temperature of the host star (dots), extracted from TEPCat orbital obliquity catalogue (Southworth 2011). The planetary radius is presented in the colour bar. The star symbol corresponds to the spin-orbit measurement of WASP-74 b. The black-dashed vertical line denotes the 6250 K effective temperature transition from Winn et al. (2010).
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.