Period analysis of the eclipsing binary U Pegasi
dc.contributor.author | Grilley, David E. | |
dc.date.accessioned | 2022-01-28T14:19:38Z | |
dc.date.available | 2022-01-28T14:19:38Z | |
dc.date.issued | 1999-04 | |
dc.description.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. | |
dc.description.department | Physics | |
dc.format | Text | |
dc.format.extent | 216 pages | |
dc.format.medium | 1 file (.pdf) | |
dc.identifier.citation | Grilley, D. E. (1999). Period analysis of the eclipsing binary U Pegasi (Unpublished thesis). Southwest Texas State University, San Marcos, Texas. | |
dc.identifier.uri | https://hdl.handle.net/10877/15231 | |
dc.language.iso | en | |
dc.subject | eclipsing binaries | |
dc.subject | observations | |
dc.title | Period analysis of the eclipsing binary U Pegasi | |
dc.type | Thesis | |
thesis.degree.department | Physics | |
thesis.degree.grantor | Southwest Texas State University | |
thesis.degree.level | Masters | |
thesis.degree.name | Master of Science |
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