| dc.contributor.advisor | Miller, Nathan A. | |
| dc.contributor.author | Wenzel, Nathan | |
| dc.date.accessioned | 2009-09-22T19:03:40Z | |
| dc.date.available | 2009-09-22T19:03:40Z | |
| dc.date.issued | 2009-04 | |
| dc.identifier.uri | http://digital.library.wisc.edu/1793/36672 | |
| dc.description | Color poster with text and diagrams. | en |
| dc.description.abstract | 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. | en |
| dc.description.sponsorship | University of Wisconsin--Eau Claire Office of Research and Sponsored Programs. | en |
| dc.language.iso | en_US | en |
| dc.relation.ispartofseries | USGZE AS589 | en |
| dc.subject | Wolf-Rayet stars--Spectra | en |
| dc.subject | O stars--Spectra | en |
| dc.subject | Stars--Spectra--Computer programs | en |
| dc.subject | Posters | en |
| dc.subject | X-ray spectroscopy--Computer programs | en |
| dc.title | X-ray Emissions of Wolf Rayet Stars. | en |
| dc.type | Presentation | en |
