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Cited article:

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

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WX Ceti: a closer look at its behaviour in quiescence and outburst

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Spectroscopic search for new SW Sextantis stars in the 3-4 h orbital period range - I

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The Nature of the Faint Chandra X-Ray Sources in the Galactic Center

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The Astrophysical Journal 640 (2) L167 (2006)
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Delays in dwarf novae II: VW Hyi, the tidal instability and enhanced mass transfer models

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The Spectra and Variability of X‐Ray Sources in a DeepChandraObservation of the Galactic Center

M. P. Muno, J. S. Arabadjis, F. K. Baganoff, et al.
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Variable Star Network: World Center for Transient Object Astronomy and Variable Stars

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Publications of the Astronomical Society of Japan 56 (sp1) S1 (2004)
https://doi.org/10.1093/pasj/56.sp1.S1

HS 2237+8154: On the onset of mass transfer or entering the period gap?

B. T. Gänsicke, S. Araujo-Betancor, H.-J. Hagen, et al.
Astronomy & Astrophysics 418 (1) 265 (2004)
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