标题： 非爆炸性氢燃烧：我们处于什么位置？ 显示英文标题

标题： Non-Explosive Hydrogen Burning: Where Do We Stand?

摘要： 核物理不确定性对冷CNO、NeNa和MgAl氢燃烧稳态模式下预测的丰度的影响，在一个简单的参数模型框架内进行了讨论。此外，这些参数计算除了能够定性地模仿详细的恒星模型预测外，还以非常清晰的方式隔离了完全源自核物理的丰度不确定性。 显示英文摘要

摘要： The impact of nuclear physics uncertaintites on the abundances predicted to emerge from the cold CNO, NeNa and MgAl modes of hydrostatic hydrogen burning is discussed in the framework of a simple parametric model. In addition of being able to mimic qualitatively detailed stellar model predictions, these parametric calculations have the virtue of isolating in a crystal-clear way abundance uncertainties of purely nuclear physics origin.