Detached cataclysmic variables are crossing the orbital period gap
Monica Zorotovic, Matthias R. Schreiber, Steven G. Parsons, Boris T., G\"ansicke, Adam Hardy, Carolina Agurto-Gangas, Ada Nebot G\'omez-Mor\'an,, Alberto Rebassa-Mansergas, Axel D. Schwope

TL;DR
This study provides strong observational evidence that detached cataclysmic variables cross the orbital period gap, supporting the disrupted magnetic braking theory of CV evolution.
Contribution
The paper offers the first strong test confirming the existence of detached CVs crossing the period gap, supporting the standard evolutionary model.
Findings
Observed an excess of detached binaries in the 2-3 hour period range.
Detected two distinct WD mass populations within the gap.
Observed a peak in the period distribution consistent with detached CVs.
Abstract
A central hypothesis in the theory of cataclysmic variable (CV) evolution is the need to explain the observed lack of accreting systems in the ~2-3 h orbital period range, known as the period gap. The standard model, disrupted magnetic braking (DMB), reproduces the gap by postulating that CVs transform into inconspicuous detached white dwarf (WD) plus main sequence (MS) systems, which no longer resemble CVs. However, observational evidence for this standard model is currently indirect and thus this scenario has attracted some criticism throughout the last decades. Here we perform a simple but exceptionally strong test of the existence of detached CVs (dCVs). If the theory is correct dCVs should produce a peak in the orbital period distribution of detached close binaries consisting of a WD and an M4-M6 secondary star. We measured six new periods which brings the sample of such binaries…
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