A more detailed look at the opacities for enriched carbon and oxygen mixtures
A more detailed look at the opacities for enriched carbon and oxygen mixtures
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DOI：
10.1111/j.1365-2966.2004.07344.x
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发表时间：
2003-10
影响因子：
4.8
通讯作者：
J. Eldridge;C. Tout
中科院分区：
文献类型：
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作者：
J. Eldridge;C. Tout
我们在恒星演化代码中包含了不透明度表，使我们能够准确地模拟由相对于太阳独立增强的碳和氧混合物组成的恒星结构。我们目前的测试，以证明新表的影响。其中两个是实际的例子：对热脉冲渐近巨星分支星星和沃尔夫-拉叶星星的演化的影响。变化很小，但可以察觉。
We have included opacity tables in our stellar evolution code that enable us to model accurately the structure of stars composed of mixtures with carbon and oxygen independently enhanced relative to solar. We present tests to demonstrate the effects of the new tables. Two of these are practical examples: the effect on the evolution of a thermally pulsing asymptotic giant branch star and a Wolf-Rayet star. The changes are small but perceptible.