the context of hot star X-rays
do the observations look like?
What trends emerge, and how
can the properties of the individual stars and of the trends among lines and
among stars be explained by the physical effects we expect might be present?
Pup: wind x-rays, but less absorption than expected
z Ori and d Ori: similar situation,
very little wind absorption; but wind-shock parameters are
Magnetic OB stars are a different story: q1 Ori C, t
Sco, g Cas
And so are normal B stars: b Cru, e
and other types of hot stars
for the future