摘要
本文采用相对论微扰法处理Ｆｅ（＋２４）系统，利用解析形式的波函数计算其低能态的能级结构及Ｋα、Ｋβ特征线（作为对比，我们也计算了Ｆｅ（＋２５）系统）．通过与现有的Ｆｅ（＋２５）Ｋα线的实验和理论比较，证明我们的方法是准确可信的，而在数学计算上则更加简便。利用这一结果，对小质量Ｘ射线密近双星的Ｆｅ（＋２４）Ｋ特征线进行了简要的定性分析．
By adopting analytic wavefunction for Fe(+24),we calculate in detail its low energy states and Kα,Kβ lines within the frame of relativistic perturbation. Compared with the results of experiments and theories on Fe(+24) Kα line by the others,our method,which is convenient for mathematical treatment,is proved to be accurate and reliable.Finally,we apply our results to LMXB systems to give a brief qualitative discussion on its Fe(+24) K feature line.
