The cataclysmic variable QZ Lib: a period bouncer
Anna F. Pala, Linda Schmidtobreick, Claus Tappert, Boris T. G\"ansicke, and Andrea Mehner

TL;DR
This study characterizes the cataclysmic variable QZ Lib, providing evidence it is a post-period minimum system with a brown dwarf donor, thus contributing to understanding the evolution of highly evolved CVs.
Contribution
The paper presents multi-epoch spectroscopic analysis of QZ Lib, confirming it as a period bouncer with a brown dwarf donor, which is a rare observational confirmation of this evolutionary phase.
Findings
Orbital period measured at 0.06436 days.
White dwarf effective temperature around 10,500 K.
Donor's temperature consistent with a T-type brown dwarf.
Abstract
While highly evolved cataclysmic variables (CVs) with brown dwarf donors, often called "period bouncers", are predicted to make up % of the Galactic CV population, only a handful of such systems are currently known. The identification and characterization of additional period bouncers is therefore important to probe this poorly understood phase of CV evolution. We investigate the evolution of the CV QZ Lib following its 2004 super-outburst using multi-epoch spectroscopy. From time-resolved spectroscopic observations we measure the orbital period of the system, d, which, combined with the superhump period d, yields the system mass ratio, . From the analysis of the spectral energy distribution we determine the structure of the accretion disc and the white dwarf effective temperature, $T_\mathrm{eff} =…
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