Fig. 6CITED IN TEXT  |  HI-RES IMAGE (165kb)  |  Previous    Next

Predicted radial velocity of rings of plasma that are stripped from the inner edge of the disk. Trajectories are shown for various inner disk radii, which sample different surface densities Σ(Rd). Inner disk radii of 10, 20, and 30 R⊙ are shown. The dashed line shows the magnitude of the Keplerian velocity for reference. The vertical line represents the nominal radius for field line accretion.