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Flickering Analysis of CH Cygni Using Kepler Data

Utilizing data from the Kepler Mission, we analyze a flickering phenomenon in the symbiotic variable star CH Cygni. We perform a spline interpolation of an averaged lightcurve and subtract the spline to acquire residual data. This allows us to analyze the deviations that are not caused by the Red Giant’s semi-regular periodic variations. We then histogram the residuals and perform moment calculations for variance, skewness, and kurtosis for the purpose of determining the nature of the flickering. Our analysis has shown that we see a much smaller scale flickering than observed in the previous literature. Our flickering scale is on the scale of fractions of a percent of the luminosity. Also, from our analysis, we are very confident that the flickering is a product of the accretion disc of the White Dwarf.

Identiferoai:union.ndltd.org:ETSU/oai:dc.etsu.edu:honors-1380
Date01 August 2016
CreatorsDingus, Thomas Holden
PublisherDigital Commons @ East Tennessee State University
Source SetsEast Tennessee State University
Detected LanguageEnglish
Typetext
Formatapplication/pdf
SourceUndergraduate Honors Theses
RightsCopyright by the authors., http://creativecommons.org/licenses/by-nc-nd/3.0/

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