Fast Hα emission line variability in RS Ophiuchi
Monthly Notices of the Royal Astronomical Society(2014)
摘要
We present optical spectroscopy of the recurrent nova RS Ophiuchi with time resolutions of ∼6, ∼5 and ∼2 min. In contrast to previous high time resolution studies of the system, changes in the emission from Hα are detected on time-scales as short as 2 min. Future high time resolution spectroscopy at a higher spectral resolution will be invaluable in determining the nature of the variation.
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关键词
binaries: symbiotic,stars: individual: RS Oph,novae, cataclysmic variables
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