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Cited article:

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Constraining Modified Gravity from Tidal Phenomena in Binary Stars

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Evolution of the Quiescent Disk Surrounding a Superoutburst of the Dwarf Nova TW Virginis

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The evolutionary status of Cataclysmic Variables: eclipse modelling of 15 systems

M McAllister, S P Littlefair, S G Parsons, et al.
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Detection of the supercycle in V4140 Sagittarii: First eclipsing ER Ursae Majoris-like object

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Global MHD Simulations of Accretion Disks in Cataclysmic Variables (CVs). II. The Relative Importance of MRI and Spiral Shocks

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SOAR observations of the high-viscosity accretion disc of the dwarf nova V4140 Sagitarii in quiescence and in outburst

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Rms–flux relation and fast optical variability simulations of the nova-like system MV Lyr

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Resolving different sources of fast X-ray variability of the dwarf nova RU Peg in quiescence★

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Monthly Notices of the Royal Astronomical Society 438 (2) 1714 (2014)
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New Method of Estimating Binary's Mass Ratios by Using Superhumps

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Taichi Kato, Akira Imada, Makoto Uemura, Daisaku Nogami, Hiroyuki Maehara, Ryoko Ishioka, Hajime Baba, Katsura Matsumoto, Hidetoshi Iwamatsu, Kaori Kubota, Kei Sugiyasu, Yuichi Soejima, Yuuki Moritani, Tomohito Ohshima, Hiroyuki Ohashi, Junpei Tanaka, Mahito Sasada, Akira Arai, Kazuhiro Nakajima, Seiichiro Kiyota, Kenji Tanabe, Kazuyoshi Imamura, Nanae Kunitomi, Kenji Kunihiro, Hiroki Taguchi, et al.
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