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On the Faint Early-time Radio and X-Ray Emissions in TDE2025aarm

  • Authors: Tatsuya Matsumoto, Tsvi Piran

Tatsuya Matsumoto and Tsvi Piran 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 4.

Multiwavelength light curves of TDE2025aarm. The purple shaded regions represent the possible X-ray light curves predicted by our models. The dashed, dotted, and solid purple curves correspond to the synchrotron (slow- and fast-cooling) and IC scenarios, respectively. The width of each curve reflects the assumed slope of the CNM density profile, k = 0.5 (thin), 1.5 (medium), and 2.5 (thick). We also show the expected radio light curves at 15 GHz (blue), which lie in the self-absorbed regime, νLν ∝ n−1/4R2. The optical light curve (red) is taken from A. Simongini et al. (2026).

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