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Polars: Long-term
light curves
Unlike disk-dominated CVs, polars tend to emit at an approximately constant level, with occasional drops to fainter levels
There is a continuum of levels, but the states tend to be called ³high², ³intermediate² and ³low²
In low states the accretion rate drops, no reservoir in a disk, so the underlying stars can become visible: important for measuring the system parameters
Feigelson, Dexter & Liller (1978)