Abstract—We critically review the results of earlier studies on magnetic stars with anomalous helium lines. We discuss the issues associated with the fossil-field theory and the scenario of the formation of magnetic stars. A special feature of the results of our study is that they are derived from more than 160 direct estimates of average surface magnetic fields Bs or models obtained by the method. The difficulty of this work is in the insufficient amount of data on He-r stars. The problem is caused by a great decrease of the v sini values of stars at the time of internal restructuring.

中文翻译：

---

具有氦异常（He-r，He-w）的磁星的演化特征和其他特征

摘要—我们批判性地回顾了先前关于氦线异常的磁星的研究结果。我们讨论了与化石场理论和磁星形成情况有关的问题。我们研究结果的一个特点是，它们是从160多个直接估计的平均表面磁场Bs或通过该方法获得的模型得出的。这项工作的困难在于He-r星的数据量不足。该问题是由于内部重组时恒星的v sin i值大大降低而引起的。