Abstract—We briefly discuss the stages of the development of high-resolution spectroscopy methods used with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, which are related to the problem considered. We consider the possibility of the multiple increase of the stellar spectroscopy efficiency as a result of application of state-of-the-art solutions in the field of adaptive optics. At the first stage, we plan to perform tasks involving the image control and correction based on the central star. This stage should be naturally started with a spectrograph with the highest spectral resolution where the relatively bright star studied can serve as the reference source in the method of adaptive optics.

摘要—我们简要讨论了与俄罗斯科学院特殊天体观测站的6米望远镜一起使用的高分辨率光谱学方法的发展阶段，这些阶段与所考虑的问题有关。我们认为，由于在自适应光学领域中应用了最新的解决方案，导致恒星光谱效率倍增的可能性。在第一阶段，我们计划执行涉及基于中央恒星的图像控制和校正的任务。这个阶段应该自然而然地从具有最高光谱分辨率的光谱仪开始，其中所研究的相对明亮的恒星可以用作自适应光学方法的参考源。