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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 12.

Overproduction factors in the ejecta relative to solar abundances, vs. mass number for models RN1 and RN2 (left), CN1 and CN2 (middle), and CN3 and CN4 (right). The color map shows the mass fractions of the different isotopes in log scale.

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