X-ray Emissions of Wolf Rayet Stars.

File(s)
Date
2009-04Author
Wenzel, Nathan
Advisor(s)
Miller, Nathan A.
Metadata
Show full item recordAbstract
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.
Subject
Wolf-Rayet stars--Spectra
O stars--Spectra
Stars--Spectra--Computer programs
Posters
X-ray spectroscopy--Computer programs
Permanent Link
http://digital.library.wisc.edu/1793/36672Description
Color poster with text and diagrams.