Ultraviolet radiation and neutrinos: two messengers from CCSNe in the CSM scenario

Silvia Gagliardini, Simone Dall'Osso, Dafne Guetta +4

Massive stars (>8 $M_{\odot }$) often undergo intense mass loss through winds or eruptive events in the final stages of their evolution, leading to the formation of a dense circumst…