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Temporal Variation in the Coronal Radius Parameter in a Jetted Tidal Disruption Event: Swift J1644+57

  • Authors: Arka Chatterjee, Kimitake Hayasaki, Prantik Nandi, Neeraj Kumari, Skye R. Heiland, Arghajit Jana, Sachindra Naik, Samar Safi-Harb

Arka Chatterjee et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 9.

Edge-on view schematic diagram of Rcor variation in the early and late stages of Swift J1644+57. The system comprises a disk around the SMBH, a corona on the disk, and a jet. The disk size is twice the tidal disruption radii, which is approximately estimated to be 2Rt ∼ 100 rg for the 106M⊙ SMBH and a solar-type star (see 1).

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