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VY sculptoris stars are magnetic cataclysmic variables

机译:vy sculptoris恒星是磁性灾难性变量

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We show that VY Scl stars must be magnetized in order to account for the absence of outbursts during their low and intermediate states. Absence of outbursts during low states requires only rather low magnetic moments but in systems in which the drops and rises of luminosity are slower than it takes for the accretion disc to adjust viscously to the variation in mass-transfer rate preventing outbursts require magnetic moments of Intermediate Polars. We discuss some evolutionary aspects of this conclusion.
机译:我们表明VY SCL星星必须磁化,以便在低低和中间状态期间缺乏爆发。在低状态期间缺乏爆发只需要相当低的磁性时刻,而是在其中滴度和亮度升高的系统中的产生慢的磁性时刻比吸积盘慢的较慢,以粘稠地调节到压差率的变化,防爆爆发需要中间的磁矩波拉。我们讨论了这一结论的一些进化方面。

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