Optical Flickering of the recurrent nova RS Ophiuchi: amplitude - flux relation
Monthly Notices of the Royal Astronomical Society(2015)
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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