Same axis layout and illustration as Figure 15, except for the case of 2M J0746+20B. Its v sin i of 33 ± 3 km s⁻¹ (Konopacky et al. 2012) is shown by the red solid line, where the dashed lines represent the errors in this measurement. We highlight the adopted radius of ∼0.96 R_J (∼0.0964 R_⊙) (Harding et al. 2013b) with the dotted green vertical track, which appears to have an equatorial inclination angle of 37 ± 4 degrees, aligned with the orbital plane of the system to within ∼5 degrees. We calculated an equatorial velocity of ∼55 km s⁻¹ which is marked by the solid blue line, in exact agreement with Harding et al. (2013b) who used the ∼2.07 hours radio period for the secondary member in their work.