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Optical Flickering of the recurrent nova RS Ophiuchi: amplitude - flux relation

Monthly Notices of the Royal Astronomical Society(2015)

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摘要
We report observations of the flickering variability of the symbiotic recurrent nova RS Oph at quiescence in five bands (UBVRI). We find evidence of a correlation between the peak-to-peak flickering amplitude (ΔF) and the average flux of the hot component (Fav). The correlation is highly significant, with a correlation coefficient of 0.85 and a p-value of ∼10−20. Combining the data from all waveba...
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关键词
accretion, accretion discs,binaries: symbiotic,stars: individual: RS Oph,novae, cataclysmic variables
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