Vockenhuber, C.; Ouellet, C O; The, L-S; Buchmann, L; Caggiano, J; Chen, A.A.; D'Auria, J.M.; Davids, B.; Fogarty, L; Frekers, D.; Wallner, Anton; Vockenhuber, C; Ruiz, C.
The nuclide 44Ti is predicted to be produced in significant quantities in core-collapse supernovae, and indeed it has been observed in the supernova remnant Cassiopeia-A by space-based γ-ray telescopes. The main production of 44Ti takes place in the α-r
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.