SPECTRAL OBSERVATIONS OF THE ALGOL - TYPE BINARY STAR δ LIBRAE

B. Rustamov, Kh. M. Mikailov, K. Alisheva, S. Mammadova, Sh. A. Agayeva, O. V. Maryeva
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Abstract

The results of spectral observations of the Algol-type binary star δ Lib are presented. The behavior of Hα and Hβ lines in the star’s spectrum during the orbital period phase is described. Based on our measurements of the radial velocities of the Hα and Hβ lines and using published data, the radial velocity curves of both components of the δ Lib system were constructed. In some phases of the orbital period, an absorption component was detected in the blue, or red, part of the Hα and Hβ line profiles. The observed Hα and Hβ absorption lines are attributed to the main component of the binary system δ Lib. It is assumed that the appearance of absorption components at these lines is associated either with suspicion of a third component in the system, or at these phases of the Hα and Hβ lines, the primary and secondary components of the δ Lib system are observed simultaneously.
双星δ天秤座的光谱观测
本文介绍了对阿尔戈尔型双星δ Lib 的光谱观测结果。描述了该恒星光谱中的 Hα 和 Hβ 线在轨道周期阶段的表现。根据我们对 Hα 和 Hβ 线径向速度的测量,并利用已公布的数据,构建了 δ Lib 系统两个组成部分的径向速度曲线。在轨道周期的某些阶段,在 Hα 和 Hβ 线剖面的蓝色或红色部分检测到了吸收成分。观测到的 Hα 和 Hβ 吸收线归因于双星系统 δ Lib 的主成分。据推测,这些吸收线出现的吸收成分要么与怀疑系统中存在第三个成分有关,要么在 Hα 和 Hβ 线的这些阶段,同时观测到 δ Lib 系统的主成分和副成分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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