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Thermal-timescale mass transfer and magnetic CVs
2004
International Astronomical Union Colloquium
AbstractWe investigate the spin evolution of the unusual magnetic CV AE Aqr. As a prototype for a potentially large population of CVs subject to a thermally unstable phase of mass transfer, understanding its future is crucial. We present a new definition of the magnetospheric radius in terms of the white dwarf's spin period, and use this along with numerical simulations to follow the spin evolution of AE Aqr. We also present preliminary SPH results suggesting the existence of a stable propeller
doi:10.1017/s0252921100001780
fatcat:d7jiaoeanvcdvdkg236tfk2hm4