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dc.contributor.advisorMiller, Nathan A.
dc.contributor.authorWenzel, Nathan
dc.descriptionColor poster with text and diagrams.en
dc.description.abstractUsing 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.en
dc.description.sponsorshipUniversity of Wisconsin--Eau Claire Office of Research and Sponsored Programs.en
dc.relation.ispartofseriesUSGZE AS589en
dc.subjectWolf-Rayet stars--Spectraen
dc.subjectO stars--Spectraen
dc.subjectStars--Spectra--Computer programsen
dc.subjectX-ray spectroscopy--Computer programsen
dc.titleX-ray Emissions of Wolf Rayet Stars.en

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