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Fig. 3


Fraction of the total mass loss contained in a cone with a semi-aperture θ given by the x-axis. The lower curve is the result for a non-rotating star losing its mass isotropically. The upper curve is for a critically rotating star (ω = 1). The intermediate dashed curves are the results of the same rotation parameter omega as in Fig. 2, i.e. ω = 0.5,   0.75,   0.9,   0.96,   0.98,   0.99, and 0.995, respectively (from bottom to top).

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