论文标题
Beta Lyrae系统中磁化空间结构的形成。 I.观察作为这种现象的研究背景
Formation of magnetized spatial structures in the Beta Lyrae system. I. Observation as a research background of this phenomenon
论文作者
论文摘要
供体磁场的发现反复构成了对现象进行彻底研究的任务，该研究基于磁场对β鸟类系统中气体结构形成和传质的过程的影响的概念。本文提供了各种长期观察结果的结果概述，分析和综合，作为进一步阐明主要针对磁化气体结构的问题的必要基础。作为这项研究的一部分，发现气态流的结构在某种程度上取决于轨道时期的阶段。因此，供体磁场会影响这些运动磁化结构的形成。在进一步的科学工作中对两个组件的质量进行分析表明，以下值是最佳的：供体的2.9 m_sun和赢得的13 m_sun。将卫星线作为某种现象的研究导致了以下事实：围绕增益器的积聚磁盘由两个部分组成：外部卫星磁盘和内部大型不透明磁盘。从对磁场的所有观察结果和研究的分析中，对6-M望远镜的观测值可被认为是最可靠的。他们形成了供体磁场的空间构型，这对于研究和理解这种相互作用系统中传质的特征很重要。有关特殊现象的磁化积聚结构的图像的进一步证据将在以下文章中提供。
The discovery of the donor magnetic field has repeatedly posed the task of a thorough study of the phenomenon, which is based on the concept of the influence of the magnetic field on the processes of the formation of gaseous structures and mass transfer in the Beta Lyrae system. This article provides an overview, analysis, and synthesis of the results of a variety of long-term observations as a necessary basis for further clarification of issues aimed primarily at the study of magnetized gaseous structures. As a part of such a study, it was found that the structure of the gaseous flows between the donor and the gainer varies in some way depending on the phases of the orbital period; and, accordingly, that the donor magnetic field influences the formation of these moving magnetized structures. The analysis of the masses of both components for use in further scientific works suggests that the following values are optimal: 2.9 M_sun for the donor and 13 M_sun for the gainer. The study of satellite lines as a certain phenomenon leads to the fact that the accretion disk surrounding the gainer consists of two parts: the external satellite disk and the internal massive opaque disk. From the analysis of all observations and studies of the magnetic field, observations on the 6-m telescope can be considered the most reliable. They have formed the spatial configuration of the donor magnetic field, which is important for studying and understanding the features of the mass transfer in this interacting system. Further evidence regarding the picture of the magnetized accretion structures as the special phenomenon will be presented in the following articles.
