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X-ray Emissions of Wolf Rayet Stars.
File(s):
- WenzelSpr09.pdf (3.680Mb PDF)
- Author(s)
- Advisor(s)
- Miller, Nathan A.
- Date
- Apr 2009
- Subject(s)
- Wolf-Rayet stars--Spectra; O stars--Spectra; Stars--Spectra--Computer programs; Posters; X-ray spectroscopy--Computer programs
- Series
- USGZE AS589
- 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.
- Description
- Color poster with text and diagrams.
- Sponsor(s)
- University of Wisconsin--Eau Claire Office of Research and Sponsored Programs.
- Permanent link
- http://digital.library.wisc.edu/1793/36672
- Export
- Export to RefWorks