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Tidal Disruption of a Magnetized Star

  • Authors: Pavel Abolmasov, Omer Bromberg, Amir Levinson, Ehud Nakar

Pavel Abolmasov et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 8.

Pressure distribution (shown by transparent gray surfaces) and magnetic field lines plotted as 3D renderings for BH 2L, t ≃ 65 days. The lower panel covers the region from x = −500 R to x = 1000 in the BH-centered system of coordinates. The upper panel shows a magnification of the central region, indicated by a green box in the lower panel.

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