Period analysis of the eclipsing binary U Pegasi
Date
1999-04
Authors
Grilley, David E.
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Abstract
Observations 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.
Description
Keywords
eclipsing binaries, observations
Citation
Grilley, D. E. (1999). Period analysis of the eclipsing binary U Pegasi (Unpublished thesis). Southwest Texas State University, San Marcos, Texas.