Speaker
Ziwei Ou
(Tsung-Dao Lee Institute, Shanghai Jiao Tong University)
Description
Starburst Galaxies (SBs) have higher star formation rate and supernova (SN) explosion rate. Therefore, SBs are promising cosmic-rays (CRs) accelerator. Such CRs produced in the birth and death of stars are expected to produce gamma-ray emission. The identification of supernova remnant and the observation of galactic-scale outflow indicate that SN-triggered activities play an important role in CR acceleration in SBs.
Primary author
Ziwei Ou
(Tsung-Dao Lee Institute, Shanghai Jiao Tong University)
