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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 5.

Three-dimensional rendering of the field lines at t = 2.4 days, i.e., stage S2. Color shows the field strength logarithm (code units), while gray contours outline the region where s = 1/2. The camera is set at an elevation of 60 deg, along the negative direction of the Y-axis. The orbit is shown with a solid green line. The straight red line is directed toward the black hole. The scale is shown by a 10 R segment in the upper part of the picture.

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