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
reasonable parameters:
t*~1 :4
to 15 times less than predicted
Ro~1.5
q~0
But, the level of wind absorption is significantly
below whatÕs expected.
And, thereÕs no significant wavelength dependence
of the optical
depth (or any parameters).