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arXiv · 1604.01103

PM J03338+3320: Long-Period Superhumps in Growing Phase Following a Separate Precursor Outburst

Taichi Kato·Enrique de Miguel·William Stein·Yutaka Maeda·Colin Littlefield·Seiichiro Kiyota·Tonny Vanmunster·Shawn Dvorak·Sergey Yu. Shugarov·Eugenia S. Kalinicheva·Roger D. Pickard·Kiyoshi Kasai·Lewis M. Cook·Hiroshi Itoh·Eddy Muyllaert
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Abstract

We observed the first-ever recorded outburst of PM J03338+3320, the cataclysmic variable selected by proper-motion survey. The outburst was composed of a precursor and the main superoutburst. The precursor outburst occurred at least 5 d before the maximum of the main superoutburst. Despite this separation, long-period superhumps were continuously seen between the precursor and main superoutburst. The period of these superhumps is longer than the orbital period by 6.0(1)% and can be interpreted to reflect the dynamical precession rate at the 3:1 resonance for a mass ratio of 0.172(4). These superhumps smoothly evolved into those in the main superoutburst. These observations provide the clearest evidence that the 3:1 resonance is triggered by the precursor outburst, even if it is well separated, and the resonance eventually causes the main superoutburst as predicted by the thermal-tidal instability model. The presence of superhumps well before the superoutburst cannot be explained by alternative models (the enhanced mass-transfer model and the pure thermal instability model) and the present observations give a clear support to the thermal-tidal instability model.

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Taichi Kato, Enrique de Miguel, William Stein, Yutaka Maeda, Colin Littlefield, Seiichiro Kiyota, Tonny Vanmunster, Shawn Dvorak, Sergey Yu. Shugarov, Eugenia S. Kalinicheva, Roger D. Pickard, Kiyoshi Kasai, Lewis M. Cook, Hiroshi Itoh, Eddy Muyllaert. 2016-04-05. PM J03338+3320: Long-Period Superhumps in Growing Phase Following a Separate Precursor Outburst. https://doi.org/10.1093/pasj%2Fpsw046

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