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Jet–Environment Interaction after Delayed Collapse in Binary Neutron Star Mergers

  • Authors: Jay V. Kalinani, Riccardo Ciolfi, Manuela Campanelli, Bruno Giacomazzo, Andrea Pavan, Allen Wen, Yosef Zlochower

Jay V. Kalinani et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 1.

3D rendering of magnetic field-line structure and rest-mass density (red-to-gray colors) for case A, at about 50 ms (left) and 75 ms (right) after merger. The inset shows a meridional view of the magnetization b2/(2ρ) at the jet base (vertical scale of up to ±250 km).

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