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. 2003 Jun 16;6(1):3. doi: 10.12942/lrr-2003-3

Figure 13.

Figure 13

Time evolution of the rotational velocity profile for a stationary, rapidly rotating relativistic star (in the Cowling approximation), using the 3rd order PPM scheme and a 1163 grid. The initial rotational profile is preserved to a high degree of accuracy, even after 20 rotational periods. (Figure 1 of Stergioulas and Font [294].)