40Ca(αγ)44Ti and the production of 44Ti in supernovae
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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.
Description
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
| Collections | ANU Research Publications |
|---|---|
| Date published: | 2008 |
| Type: | Journal article |
| URI: | http://hdl.handle.net/1885/81906 |
| Source: | Journal of Physics G: Nuclear and Particle Physics |
| DOI: | 10.1088/0954-3899/35/1/014034 |
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| File | Description | Size | Format | Image |
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| 01_Vockenhuber_40Ca(αγ)44Ti_and_the_2008.pdf | 206.86 kB | Adobe PDF | Request a copy |
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