Period analysis of the eclipsing binary U Pegasi

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dc.contributor.authorGrilley, David E.
dc.date.accessioned2022-01-28T14:19:38Z
dc.date.available2022-01-28T14:19:38Z
dc.date.issued1999-04
dc.description.abstractObservations of the W Ursae Majoris type binary U Pegasi were taken over 5 nights in October/November 1995. Numerical techniques were used to generate a period and an epoch of primary minimum. The method and results are compared to previous studies of U Pegasi for verification. The methods used generate results within observational error limits of previous observations. These current computer techniques invite consideration as a new paradigm for standard period determination for eclipsing binary systems.
dc.description.departmentPhysics
dc.formatText
dc.format.extent216 pages
dc.format.medium1 file (.pdf)
dc.identifier.citationGrilley, D. E. (1999). Period analysis of the eclipsing binary U Pegasi (Unpublished thesis). Southwest Texas State University, San Marcos, Texas.
dc.identifier.urihttps://hdl.handle.net/10877/15231
dc.language.isoen
dc.subjecteclipsing binaries
dc.subjectobservations
dc.titlePeriod analysis of the eclipsing binary U Pegasi
dc.typeThesis
thesis.degree.departmentPhysics
thesis.degree.grantorSouthwest Texas State University
thesis.degree.levelMasters
thesis.degree.nameMaster of Science

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