X-ray Emissions of Wolf Rayet Stars.
Miller, Nathan A.
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Using a program called Spect 3D, control models of O-stars, specifically Zeta Puppis, were created and then compared with models of Wolf-Rayet stars. The models were made in a similar fashion comprising a three region shell surrounding the star consisting of a warm region followed by the shock region of the stellar wind and finishing with another warm region. The X-ray emissions of the winds were compared for these two types of stars.
X-ray spectroscopy--Computer programs
Color poster with text and diagrams.