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Fig. 8.


Visibilities of the l = 0 through l = 3 modes for the G2 star as a function of inclination angle and equatorial rotation velocity for the case with 0 G and using the 6173 Å line. For clarity the values have been divided by the visibility of the corresponding m = 0 mode at i = 0°. The corresponding values, which are not shown, go up to 0.02, but are generally less than 0.01.

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