Loaded layer-cake model for cosmic ray interaction around exploding super-giant stars making black holes

Documenti analoghi

• Cosmic ray contributions from rapidly rotating stellar mass black holes: Cosmic Ray GeV to EeV proton and anti-proton sources
  di: Allen, M. L., et al.
  Pubblicazione: (2024)
• A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies
  di: Allen, M. L., et al.
  Pubblicazione: (2025)
• SVOM GRB 250314A at z $\simeq$ 7.3: an exploding star in the era of reionization
  di: Cordier, B., et al.
  Pubblicazione: (2025)
• Where do stars explode in the ISM? -- The distribution of dense gas around evolved massive stars in M33
  di: Sarbadhicary, Sumit K., et al.
  Pubblicazione: (2023)
• The influence of rotation and metallicity on the explodability of massive stars
  di: Luo, Renyu, et al.
  Pubblicazione: (2025)