Multi-color light curves of TCP J23580961+5502508 reveal early superhumps with a shift from single to two-armed flaring in the accretion disk during the initial rise of the superoutburst.
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A moderate factor of 2-3 reduction in magnetic braking efficiency at the fully convective boundary suffices to reproduce key features of cataclysmic variable evolution when using an updated saturated prescription.
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A growth of early superhump: Multi color observation of the WZ Sge star TCP J23580961+5502508
Multi-color light curves of TCP J23580961+5502508 reveal early superhumps with a shift from single to two-armed flaring in the accretion disk during the initial rise of the superoutburst.
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A modest change in magnetic braking at the fully convective boundary explains cataclysmic variable evolution
A moderate factor of 2-3 reduction in magnetic braking efficiency at the fully convective boundary suffices to reproduce key features of cataclysmic variable evolution when using an updated saturated prescription.