dc.contributor.advisor | Miller, Nathan A. | |
dc.contributor.author | Vasel, Justin A. | |
dc.contributor.author | McGill, Gregory J. | |
dc.date.accessioned | 2011-11-30T14:30:20Z | |
dc.date.available | 2011-11-30T14:30:20Z | |
dc.date.issued | 2011-05 | |
dc.identifier.uri | http://digital.library.wisc.edu/1793/55358 | |
dc.description | Color poster with diagrams, images, and charts. | en |
dc.description.abstract | Although it is well known that O and B type stars are X-ray emitters, the mechanism driving this process is not entirely understood. Knowing
the radial location of the X-ray emission is key to understanding which models of X-ray emission are correct. In this project, several photospheric models were analyzed to determine which should be used and reconciled discrepancies
within the model with observational data of the B-type star, Spica. | 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 | X-ray sources, Galactic | en |
dc.subject | X-ray spectroscopy | en |
dc.subject | Stellar photospheres | en |
dc.subject | B stars--Spectra | en |
dc.subject | Posters | en |
dc.title | Determining the Radial Location of the X-ray Emitting Zones of Spica | en |
dc.type | Presentation | en |