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dc.contributor.advisorHerczeg, Tibor J.,en_US
dc.contributor.authorMccartney, Scott Alan.en_US
dc.date.accessioned2013-08-16T12:30:44Z
dc.date.available2013-08-16T12:30:44Z
dc.date.issued1999en_US
dc.identifier.urihttps://hdl.handle.net/11244/5876
dc.description.abstractThe light curves of W Ursae Majoris stars often show asymmetries which are called the O'Connell Effect. Traditionally, these asymmetries were measured by calculating the magnitude difference of the peak intensity at each of the light curve maxima. These asymmetries are usually modeled with ad hoc spots, usually considered as magneto-hydrodynamic in origin. The work of Zhou and Leung offers a thermodynamically motivated solution for these light curve asymmetries, based on a dynamic model for the system. The results presented here are derived from a simple model using Zhou and Leung's theory. These models are then compared to a database of W Ursae Majoris systems that have published photometric solutions.en_US
dc.description.abstractAdditionally two new parameters for measuring light curve asymmetry are developed: the O'Connell Effect Ratio and the Light Curve Asymmetry. These new parameters are calculated from the observational photometry and from the theoretical models.en_US
dc.format.extentix, 152 leaves :en_US
dc.subjectWolf-Rayet stars.en_US
dc.subjectA stars.en_US
dc.subjectDouble stars.en_US
dc.subjectPhysics, Astronomy and Astrophysics.en_US
dc.titleA 2-D model for the O'Connell effect in W Ursae Majoris systems /en_US
dc.typeThesisen_US
dc.thesis.degreePh.D.en_US
dc.thesis.degreeDisciplineHomer L. Dodge Department of Physics and Astronomyen_US
dc.noteSource: Dissertation Abstracts International, Volume: 60-11, Section: B, page: 5565.en_US
dc.noteAdviser: Tibor J. Herczeg.en_US
ou.identifier(UMI)AAI9949702en_US
ou.groupCollege of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy


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