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Norton, A. J.; Somerscales, R. V.; Parker, T. L.; Wynn, G. A. and West, R. G.
(2004).
URL: http://www.astroscu.unam.mx/~rmaa/rmsc20_frameset....
Abstract
We present the results of simulations that explore the variety of accretion flows possible in magnetic cataclysmic variables (mCVs). Our simulations evolve to equilibrium periods spanning 0.01 < P[spin]/P[orb] < 0.6 and the resulting flows vary from disc-fed systems at P[spin]/P[orb] ˜ 0.01 - 0.1, to stream fed systems at P[spin]/P[orb] ˜ 0.1 - 0.5 and systems fed from a ring at the outer edge of the white dwarf's Roche lobe at P[spin]/P[orb] ˜ 0.6.