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The HU Aqr planetary system hypothesis revisited

Monthly Notices of the Royal Astronomical Society(2015)

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摘要
We study the mid-egress eclipse timing data gathered for the cataclysmic binary HU Aquarii during the years 1993–2014. The (O−C) residuals were previously attributed to a single ∼7 Jupiter mass companion in ∼5 au orbit or to a stable two-planet system with an unconstrained outermost orbit. We present 22 new observations gathered between 2011 June and 2014 July with four instruments around the worl...
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关键词
techniques: photometric,stars: individual: HU Aqr,novae, cataclysmic variables,planetary systems
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