Modeling of the galactic distribution of 44Ti emitting young supernova remnants
Following the lone detection of the Galactic supernova remnant Cas A by gamma-ray detectors aboard CGRO and hard X-ray detectors aboard INTEGRAL in the nuclear lines of the 44Ti decay chain, The et al, 2006, argued that these surveys should have detected several sources, given models for the yield o...
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| Format: | Others |
| Language: | en |
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McGill University
2012
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| Online Access: | http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=107867 |