Weber and Davis revisited: Mass losing rotating magnetic winds

The original Weber and Davis theory for the rotating magnetic solar wind is correct only in the case of zero photospheric mass loss. We have extended this theory to the case of nonzero photospheric mass loss, and we show how prior applications of the theory to the mass losing early-type stars are in conceptual and numerical error. One surprising result is that the azimuthal velocity structure may be affected in an interesting nonintuitive way