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arXiv · 2312.00307

VLBI detection of the AE Aqr twin, LAMOST J024048.51+195226.9

Pengfei Jiang·Lang Cui·Xiang Liu·Bo Zhang·Yongfeng Huang·Hongmin Cao·Tao An·Jun Yang·Fengchun Shu·Guiping Tan·Jianping Yuan
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Abstract

LAMOST J024048.51+195226.9 (J0240+1952) was recently identified as the second AE Aquarii (AE Aqr)-type cataclysmic variable, possessing the fastest known rotating white dwarf. We performed a Very Long Baseline Interferometry (VLBI) observation of J0240+1952 utilizing the European VLBI Network at 1.7\,GHz, to obtain the first view of the radio morphology on mas scale. Our high-resolution VLBI image clearly shows that the radio emission is compact on mas scale ($\lesssim2$\,AU), with no evidence for a radio jet or extended emission. The compact radio source has an average flux density of $\sim0.37$\,mJy, and its brightness temperature is given at $\gtrsim2.3\times10^{7}$\,K, confirming a non-thermal origin. The emission exhibits irregular variations on a time-scale of tens of minutes, similar to the radio flares seen in AE Aqr. The measured VLBI position of J0240+1952 is consistent with that derived from \textit{Gaia}. Our results favour the model in which the radio emission is attributed to a superposition of synchrotron radiation from expanding magnetized blobs of this system.

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Pengfei Jiang, Lang Cui, Xiang Liu, Bo Zhang, Yongfeng Huang, Hongmin Cao, Tao An, Jun Yang, Fengchun Shu, Guiping Tan, Jianping Yuan. 2023-12-01. VLBI detection of the AE Aqr twin, LAMOST J024048.51+195226.9. https://doi.org/10.1093/mnrasl%2Fslad178

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