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Hyperactive Magnetar Eruptions: Giant Flares, Baryon Ejections, and Fast Radio Bursts

  • Authors: Ashley Bransgrove, Andrei M. Beloborodov, Yuri Levin

Ashley Bransgrove et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 2.

Magnetic field evolution of the hyperactive magnetar. Four snapshots are shown at times t = 0, 200​​​​​​, 500​​​​​​, and 700 yr. The green curves represent poloidal magnetic field lines. The top row shows ﹩{B}_{\phi }/(r\sin \theta )﹩. The bottom row shows the log of baryon density ρ in units of g cm−3. In each panel, the horizontal x-axis shows the distance from the vertical z-axis (the axis of symmetry); both x and z are in units of 10 km. The inner and outer dashed white curves are contours of ρ = ρcore and ρ = ρdrip. The animation of this figure shows the sequence from t = 0–700 yr. The animation real-time duration is 15 s.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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