Calendar

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Gruppi Corso MHD 10:00
Gruppi Corso MHD
Gen 13@10:00–11:00
Preparazione per l’esame del corso Magnetohydrodynamics in Astrophysical Processes
Visita studenti Accademia Belle Arti (Porf. Fraia) 10:00
Visita studenti Accademia Belle Arti (Porf. Fraia)
Gen 13@10:00–12:00
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Visita Museo 15 persone (prof. Chimica Unipa) 10:30
Visita Museo 15 persone (prof. Chimica Unipa)
Gen 15@10:30–13:00
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Meeting EXOPA 9:30
Meeting EXOPA
Gen 20@9:30–10:30
 
Seminario: Salvatore Orlando (INAF-OAPa) 15:00
Seminario: Salvatore Orlando (INAF-OAPa)
Gen 20@15:00–16:00
Abstract: Core-collapse supernova remnants (SNRs) offer a powerful diagnostic of massive-star evolution and explosion physics. Their complex morphologies and chemical inhomogeneities retain signatures of the supernova (SN) engine, including asymmetries, nucleosynthetic yields, and compact-object formation. In young remnants (<5000 years), the debris still preserves this early “memory”, while the large-scale structure reflects interactions with the circumstellar medium (CSM) shaped by
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