"From the thermonuclear supernova to the supernova remnant"

Résumé

Outline:

1. Structure and dynamics of a young shell SNR: What shapes the ejecta in the remnant phase
2. Typing and sub-typing SNRs: How to tell apart thermonuclear from core-collapse, and can we do more?
3. Toward a grid of SN-SNR models: Using the output from SN models as input for SNR simulations (N100, N grid, D6)