Abstract

The paper presents the first results of the ongoing spectropolarimetric monitoring of magnetic fields of stars, whose chemically peculiar nature has been previously revealed with the 1-m SAO RAS telescope. We selected the sample candidates using the photometric data of the Kepler and TESS space missions. The efficiency of the method of searching for new CP stars based on photometric light curves has been confirmed. We present the magnetic field measurements and estimate the atmospheric parameters of the objects under study.

中文翻译：

---

开普勒任务数据发现新 CP 星的磁场

摘要

该论文介绍了正在进行的恒星磁场光谱偏振监测的第一个结果，其化学奇特性质之前已由 1 米 SAO RAS 望远镜揭示。我们使用开普勒和 TESS 太空任务的光度数据选择了候选样本。基于光度光变曲线寻找新CP星的方法的有效性已得到证实。我们提出了磁场测量结果并估计了所研究物体的大气参数。