Physics
Scientific paper
May 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..nws.c1013t&link_type=abstract
American Physical Society, 8th Annual Meeting of the APS Northwest Section, May 18-20, 2006, abstract #C1.013
Physics
Scientific paper
We report results from summer 2005 in an ongoing study of the eclipsing binary star system: 44i-Bootes. Light curves, representing the intensity of illumination received from the system over the course of a night were measured for a number of clear nights. The observation system has been improved with the introduction of a computer-guided 16" Ritchie-Chretien reflector. From this data, the time of eclipse is inferred. The period between eclipses has been slowly increasing since observations began, nearly a century ago. Residuals computed after the lengthening period is taken into account suggest an oscillation with a 60+ year period.
Henderson Scott
Olsen Thomas
Sugaya Satomi
Thompson Christina
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