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Reconnection-driven Plasma Loading for Prompt Emission in Tidal Disruption Event Jets

  • Authors: Rin Oikawa, Yuri Sato

Rin Oikawa and Yuri Sato 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 3.

Predicted flux from magnetic reconnection in the vicinity of the BH for a TDE at z ∼ 0.01. The red shaded regions correspond to reconnection rates of βrec = 0.1 (collisionless regime; upper curve) and βrec = 0.01 (collisional regime; lower curve), respectively. The black curve shows the sensitivity of AMEGO for an exposure time of 106 s (J. McEnery et al. 2019). The predicted MeV gamma-ray emission is expected to precede the prompt emission (see Figure 2).

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