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56Ni Production in Long-lived Binary Neutron Star Merger Remnants

  • Authors: Maximilian Jacobi, Fabio Magistrelli, Eleonora Loffredo, Giacomo Ricigliano, Leonardo Chiesa, Sebastiano Bernuzzi, Albino Perego, Almudena Arcones

Maximilian Jacobi et al 2026 The Astrophysical Journal Letters 999 .

  • Provider: AAS Journals

Caption: Figure 4.

γ-ray emission spectrum at t = 7 days for BLh_q1.49 at 40 Mpc for a polar (upper panel) and an equatorial (lower panel) viewing angle. Colored lines and arrows on top of the panels indicate the contribution of individual isotopes and the original line positions, respectively. Gray lines show the sensitivity of the NuStar, COSI, e-ASTROGRAM, and GammaTPC telescopes.

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