恰当 发表于 2025-3-21 19:16:08
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Nuclear Reaction Rates,the star shine. These reactions transform lighter nuclei into heavier nuclei and produce energy as long as the binding energy per nucleon of the reacting particles is smaller than the binding energy per nucleon of the product of the reactions.macrophage 发表于 2025-3-22 01:20:57
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Final Stages of Single Star Evolution, for a next burning phase if the temperature is high enough. The maximum temperature that can be attained in the stellar interior depends largely on the total mass of the star. It depends also on this temperature whether or not the produced ‘ashes’ will be ignited for a subsequent nuclear fusion phase.碎石头 发表于 2025-3-22 15:28:38
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Structure and Evolution of Single and Binary Stars978-94-011-2502-4Series ISSN 0067-0057 Series E-ISSN 2214-7985Camouflage 发表于 2025-3-23 04:25:22
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