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Fig. 7


Spatial and temporal variations of log density, radial velocity, and lateral velocity for a modelwith stellar rotation at the surface vy = 300 km s−1 (see text), with color-coding as in Figs. 2 and 4. The vertical variation in this simulation extends only from 1.0 to 1.5 R* , but the lateral variation is displayed as before over twice the horizontal box length 0.1R* . From left to right are shown the time evolution over 350 ks after the CAK initial condition, in steps of 50 ks.

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