Classifying Optical (Out)bursts in Cataclysmic Variables: The Distinct Observational Characteristics of Dwarf Novae, Micronovae, Stellar Flares, and Magnetic Gating

K. Iłkiewicz, Simone Scaringi, Martina Veresvarska, D. de Martino, Colin Littlefield, Christian Knigge, J. Paice, Anwesha Sahu
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Abstract

Cataclysmic variables can experience short optical brightenings, which are commonly attributed to phenomena such as dwarf novae outbursts, micronovae, donor flares, or magnetic gating bursts. Since these events exhibit similar observational characteristics, their identification has often been ambiguous. In particular, magnetic gating bursts and micronovae have been suggested as alternative interpretations of the same phenomena. Here we show that the timescales and energies separate the optical brightenings into separate clusters consistent with their different classifications. This suggests that micronovae and magnetic gating bursts are in fact separate phenomena. Based on our findings, we develop diagnostic diagrams that can distinguish between these bursts/flares based on their properties. We demonstrate the effectiveness of this approach on observations of a newly identified intermediate polar, CTCV J0333-4451, which we classify as a magnetic gating system. CTCV J0333-4451 is the third highest spin-to-orbital period ratio intermediate polar with magnetic gating, suggesting that these bursts are common among these rare systems.
大灾变变星的光学(爆发)分类:矮新星、微新星、恒星耀斑和磁门的不同观测特征
大灾变变星会出现短暂的光学增亮,这通常被归因于矮新星爆发、微新星、供体耀斑或磁门爆发等现象。由于这些事件表现出相似的观测特征,它们的识别往往很模糊。特别是磁门暴和微新星被认为是对同一现象的另一种解释。在这里,我们证明了时间尺度和能量将光学增亮分为不同的群组,这与它们的不同分类是一致的。这表明微子星和磁门脉冲串实际上是不同的现象。根据我们的发现,我们绘制了诊断图,可以根据这些爆发/耀斑的特性对它们进行区分。我们在对一个新发现的中间极--CTCV J0333-4451的观测中证明了这种方法的有效性,我们将其归类为磁栅极系统。CTCV J0333-4451是自旋轨道周期比第三高的磁门控中间极,这表明这些爆发在这些罕见的系统中很常见。
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