|Title (1st Abstract)||
The spectacular evolution of Supernova 1996al over 15 years: a low energy explosion of a stripped massive star in a highly structured environment
INAF – Osservatorio Astronomico di Padova (Italy)
10. SNe and SNRs with circumstellar interactions
The final fate of massive stars is not well explored and depending on the stellar mass may have very much different outputs, ranging from very energetic explosions (e.g. GRB-SNe) to direct collapse on black-holes with very weak or not explosion at all (Heger, Woosley, & Baraffe, 2005).
INAF-Osservatorio Astronomico di Padova