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Multicolor Photometry of 1SWASP J162117.36+441254.2 during the 2016 Outburst

机译:1SWASP J162117.36 + 441254.2的多色测光测量在2016年爆发期间

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We present preliminary results of BVRcIc photometric observations of 1SWASP J162117.36+441254.2 during the 2016 outburst. Observations were carried out at 1.25-m telescope located in Crimean Astrophysical Observatory. Previously this star was thought as eclipsing variable of the W UMa-type until the outburst, but with the help of numerous worldwide observations this object was classified as the long-term dwarf nova. Our findings demonstrate the dramatic changes of the light curves profile in all color bands during the outburst. This can be interpreted as the presence of erupted accretion disk at the early stages of outburst and the emergence of ellipsoid effect of the secondary component of the system at a later stage.
机译:我们在2016年爆发期间提出了1SWASP J162117.36 + 441254.2的BVrcic光度观测的初步结果。在位于克里米亚半岛天体物理观测所的1.25米的望远镜下进行观察。此前,这颗恒星被认为是W UMA型的黯然失色变量,直到爆发,但在许多全球观察的帮助下,该目的被归类为长期矮人新星。我们的研究结果表明了在爆发期间所有色带中的光曲线曲线的戏剧性变化。这可以被解释为在突出的早期阶段的爆发磁盘的存在和稍后阶段在稍后阶段的次要组分的椭球效应的出现。

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