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dc.contributor.advisorMiller, Nathan A.
dc.contributor.authorVasel, Justin A.
dc.contributor.authorMcGill, Gregory J.
dc.date.accessioned2011-11-30T14:30:20Z
dc.date.available2011-11-30T14:30:20Z
dc.date.issued2011-05
dc.identifier.urihttp://digital.library.wisc.edu/1793/55358
dc.descriptionColor poster with diagrams, images, and charts.en
dc.description.abstractAlthough 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.sponsorshipUniversity of Wisconsin--Eau Claire Office of Research and Sponsored Programsen
dc.language.isoen_USen
dc.relation.ispartofseriesUSGZE AS589en
dc.subjectX-ray sources, Galacticen
dc.subjectX-ray spectroscopyen
dc.subjectStellar photospheresen
dc.subjectB stars--Spectraen
dc.subjectPostersen
dc.titleDetermining the Radial Location of the X-ray Emitting Zones of Spicaen
dc.typePresentationen


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    Posters of collaborative student/faculty research presented at CERCA

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