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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 4.

Mean density (normalized by ﹩{\rho }_{{\rm{BH}}}={M}_{{\rm{BH}}}{r}_{* }^{-3}﹩) within the stellar debris (tracer condition s > 0.5) as a function of radial coordinate r* of the stellar center of mass throughout the simulation stages S1 and S2. Color indicates the time measured from the beginning of the simulation.

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