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Lecture 9 Hydrogen Burning Nucleosynthesis, Classical Novae, and X-Ray Bursts

Lecture 9 Hydrogen Burning Nucleosynthesis, Classical Novae, and X-Ray Bursts. Once the relevant nuclear physics is known in terms of the necessary rate factors, l = N A < s v >, the composition can be solved from the coupled set of rate equations:.

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Lecture 9 Hydrogen Burning Nucleosynthesis, Classical Novae, and X-Ray Bursts