O Star Giant Bubbles in M33
M.S. Oey & P. Massey
We have studied two remarkable, giant (130 pc diameter) H-alpha bubble
nebulae in M33, and have spectroscopically identified a single,
dominant O9 star centrally located in each. We compare the nebular
parameters with those predicted by analytical models of wind-blown
bubbles, taking into account the evolution of wind power from the
parent stars. The agreement is good, suggesting that these objects
provide a compelling record of the effect that individual, normal OB
stars have on the interstellar medium. The study of such nebulae can
provide insight on the evolution of the parent star and its winds.
1994 ApJ 425, 635
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