[PDF][PDF] Modelling the 𝜸-ray emission from 𝜼 Carinae
M Balbo, R Walter - 2023 - inspirehep.net
Colliding winds of massive stars in binary systems (CWB) have been proposed as potential
sites of relativistic cosmic-ray acceleration and non-thermal very-high-energy (VHE) photons …
sites of relativistic cosmic-ray acceleration and non-thermal very-high-energy (VHE) photons …
[PDF][PDF] Modelling the 𝜸-ray emission from 𝜼 Carinae
M Balbo, R Walter - 2023 - pos.sissa.it
Colliding winds of massive stars in binary systems (CWB) have been proposed as potential
sites of relativistic cosmic-ray acceleration and non-thermal very-high-energy (VHE) photons …
sites of relativistic cosmic-ray acceleration and non-thermal very-high-energy (VHE) photons …