Determining the Radial Location of the X-ray Emitting Zones of Spica
Vasel, Justin A.
McGill, Gregory J.
Miller, Nathan A.
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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.
X-ray sources, Galactic
Color poster with diagrams, images, and charts.