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15:30
Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of supernova remnants | Salvatore Orlando ( INAF- Osservatorio Astronomico di Palermo)
@ Aula OAPA
Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of supernova remnants | Salvatore Orlando ( INAF- Osservatorio Astronomico di Palermo)
@ Aula OAPA
Jul 27 @ 15:30 – 16:30
The thermal structure of the post-shock region of a young supernova remnant (SNR) is heavily affected by two main physical effects, namely the back-reaction of accelerated cosmic rays and the Rayleigh-Taylor instabilities developing at the contact discontinuity between the ejecta and the shocked interstellar medium (ISM). In this contribution, we investigate the role played by both physical mechanisms in the
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