标题： β CrB 的能量分布对于特定的恒星丰度 显示英文标题

标题： The energy distribution of beta CrB for the specific stellar abundances

摘要： β CrB的观测和计算的能量分布比较表明，具有恒星特定化学成分的模型可以解释可见光能量分布，但仍然无法再现1700 A以短波的紫外线观测。 此外，强Fe II和Mg II紫外线吸收线的预测吸收量远大于观测值。 显示英文摘要

摘要： The comparison of the observed and computed energy distributions of beta CrB has shown that a model with the specific chemical composition of the star can account for the visual enery distribution, while it is still unable to reproduce ultraviolet observations shortward of 1700 A. Furthermore, the predicted absorption of strong Fe II and Mg II UV lines is much larger than the observed one.