We carefully consider observational and theoretical constraints on the global properties of
secondary stars in cataclysmic variable stars (CVs). We then use these constraints to …

We discuss the properties of 137 cataclysmic variables (CVs) which are included in the
Sloan Digital Sky Survey (SDSS) spectroscopic data base, and for which accurate orbital …

We report on successes and failures in searching for positive superhumps in cataclysmic
variables, and show the superhumping fraction as a function of orbital period. Basically, all …

We present a systematic survey for mass-transferring and recently detached cataclysmic
variables (CVs) with evolved secondaries, which are progenitors of extremely low mass …

We present a catalogue of 507 cataclysmic variables (CVs) observed in SDSS I to IV
including 70 new classifications collated from multiple archival data sets. This represents the …

The 28 cataclysmic variables (CVs) found in 2005 in the Sloan Digital Sky Survey are
presented with their coordinates, magnitudes, and spectra. Five of these systems are …

We present a binary evolution study of cataclysmic variables (CVs) and related systems with
white dwarf (WD) accretors, including for example, AM CVn systems, classical novae …

Of more than a thousand known cataclysmic variables (CVs), where a white dwarf is
accreting from a hydrogen-rich star, only a dozen have orbital periods below 75 minutes …

We report the discovery of ZTF J0127+ 5258, a compact mass-transferring binary with an
orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely …

ABSTRACT AM CVn systems are ultra-compact, hydrogen-depleted, and helium-rich,
accreting binaries with degenerate or semidegenerate donors. We report the discovery of …