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High-resolution Simulations of the Interaction between the Nova/Supernova Ejecta and the Accretion Disk

  • Authors: Axel S. Lechuga, Domingo García-Senz, Jordi José

Axel S. Lechuga et al 2025 The Astrophysical Journal 992 .

  • Provider: AAS Journals

Caption: Figure 14.

Top left panel: relaxation process, which consists in resetting the velocities every 100 iterations with the aim of reducing kinetic energy noise. Top right panel: complete relaxation process for t several times the collision time. Bottom panel: post-relaxed density profile of the accretion disk in models CN2, CN3, and CN4.

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