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Outflow–Cloud Interaction as the Possible Origin of the Peculiar Radio Emission in the Tidal Disruption Event AT2018cqh

  • Authors: Lei Yang, Xinwen Shu, Guobin Mou, Yongquan Xue, Luming Sun, Fabao Zhang, Zhumao Zhang, Yibo Wang, Tao Wu, Ning Jiang, Hucheng Ding, Tinggui Wang

Lei Yang et al 2025 The Astrophysical Journal Letters 993 .

  • Provider: AAS Journals

Caption: Figure 1.

Natural-weighted images of VLBA observations of AT2018cqh at three frequencies. In each image, the bottom right ellipse is the shape of the restoring beam, with sizes of 14.51 × 5.29 mas for the L band, 3.20 × 1.30 mas for the C band, and 1.99 × 0.81 mas for the X band, respectively. The contour levels are 2.5σ × (−1, 1, 2, 4, 8) for the L band and 2.5σ × (−1, 1, 2, 4, 8, 16, 32, and 64) for the C band and X band.

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