Speaker
Dr
Yerlan Aimuratov
(Fesenkov Astrophysical Institute)
Description
Observations of supernovae (SNe) Ic occurring after the prompt emission of long gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model, where GRBs originate from a binary composed of 10 solar masses carbon–oxygen (CO) star and a neutron star (NS). We report on recent progress in understanding the phenomenon and draw some prospects on GRB-SN research.
Author
Dr
Yerlan Aimuratov
(Fesenkov Astrophysical Institute)