40Ca(αγ)44Ti and the production of 44Ti in supernovae
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
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|Source:||Journal of Physics G: Nuclear and Particle Physics|
|01_Vockenhuber_40Ca(αγ)44Ti_and_the_2008.pdf||206.86 kB||Adobe PDF||Request a copy|
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