Line γ-ray emission from supernovae and supernova remnants Original Research Article

We have calculated line γ-ray emission from supernovae and supernova remnants with various explosion models and nucleosynthesis for both thermonuclear supernovae (SNe Ia) and core collapse supernovae (SNe Ib, Ic, II-P). The calcualted line γ-ray light curves are strongly model dependent, thus both γ-ray observations and theoretical study of supernovae and young supernova remnants are very important.