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).