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Detection of Short Fading Episodes in Two Dwarf Novae from VSNET Observations

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VY Sculptoris stars as magnetic cataclysmic variables

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SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h

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Dynamical masses of a nova-like variable on the edge of the period gap

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Dwarf nova-type cataclysmic variable stars are significant radio emitters

Deanne L. Coppejans, Elmar G. Körding, James C. A. Miller-Jones, et al.
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The Identification of Hydrogen-deficient Cataclysmic Variable Donor Stars

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The Astrophysical Journal 861 (2) 102 (2018)
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ABUNDANCE DERIVATIONS FOR THE SECONDARY STARS IN CATACLYSMIC VARIABLES FROM NEAR-INFRARED SPECTROSCOPY

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Delays in dwarf novae I: The case of SS Cygni

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ASAS J071404+7004.3 – a close, bright nova-like cataclysmic variable with gusty winds

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