Lines are well fit by our four parameter model (b is actually held constant at b=1; so three free parameters): z PupÕs X-ray lines are consistent with a spatially
distributed, spherically symmetric, radially accelerating wind scenario, with
to 15 times less than predicted
But, the level of wind absorption is significantly
below whatÕs expected.
And, thereÕs no significant wavelength dependence
of the optical
depth (or any parameters).