The short spindown timescale of AE Aqr requires a high birthrate for such systems, implying that a substantial fraction of cataclysmic variables must have formed in this way. A simple estimate suggests that this fraction could be of order one-third of current CVs. We emphasize the importance ...
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We present 14 nights of medium resolution (1-2\\AA) spectroscopy of the\neclipsing cataclysmic variable UU Aquarii obtained during a high accretion\nstate in 1995 August-October. UU Aqr appears to be an SW Sextantis star, as\nnoted by Baptista, Steiner, & Horne (1996), and we discuss...
Since both the density and the scale are incompatible with a standard post-shock accretion column of a mCV, the hot plasma in AE Aqr cannot be a product of mass accretion onto the white dwarf. The widths of the H-like Kα emission (=Lyα) lines of N and O, on the other hand, ...
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