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The top documents tagged [core h]
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The s-process Fe Co Ni Rb Ga Ge Zn Cu Se Br As Zr Y Sr Kr (n, ) ()() ()() r-process p-process 63 Ni, t 1/2 =100 a 64 Cu, t 1/2 =12 h, 40 % (
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Stellar Evolution – the Life and Death of a Star…
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Our sun does not have a solid surface. Most of the energy comes from the core
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Activity #32, pages 111-112 (pages 109-110 were done last Friday)
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Memory restriction, limits and heterogeneous grids. A case study. Txema Heredia Or an example of how to adapt your policies to your needs
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The Sun
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