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
R o~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).