| 氢燃烧后的恒星演化及物理原理 |
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| 引用本文： | 彭秋和.氢燃烧后的恒星演化及物理原理[J].紫金山天文台台刊,1994,13(1):60-61. |
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| 作者姓名： | 彭秋和 |
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| 摘 要： | This is a review talk. The first part of the talk is to introduce briefly the evolutionary picture of stars with various mass after hydrogen burning. The second one of the talk is about some important physical factors affected on the stellar evolution. The content of the second part of the talk is as follows: A) Physics controlling nuclear burning in the stars 1. Ignition temprature of nuclear burning 2. Lower limit on the core mass of stars for igniting nuclear burning
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| 关 键 词： | 恒星演化 物理原理 氢燃烧 |
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