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射电星系喷流准直机制研究进展
Alternative TitleProgress in the Study of the Jet Collimation Mechanism of Radio Galaxies
沈玉玲1; 崔朗1; 安涛2; 刘祥1
2022-03-01
Source Publication天文学进展
ISSN1000-8349
Volume40Issue:1Pages:18-36
Contribution Rank1
Abstract射电星系是射电噪活动星系核(AGN)的一个重要子类,相对论性的射电喷流是其典型的观测特征之一。射电喷流的加速过程、准直机制以及磁场所起的作用一直是天文学家关注的重点。近年来,随着高分辨率VLBI观测技术的发展,利用射电天文观测仪器已经能够探测到AGN核心区域,从而能够研究喷流的内部结构和物理过程。得益于此,天文学家在近邻射电星系喷流准直机制的观测研究方面取得了重大进展。首先介绍了主流的喷流形成模型,之后通过典型的研究案例,对FR-I和FR-II两类射电星系准直机制研究的最新进展进行阐述,最后对射电星系喷流准直机制研究进行了总结和展望。
Other AbstractRadio galaxies are an important subclass of radio-loud active galactic nuclei(AGN),and relativistic radio jets are one of its typical observational features.The acceleration process of radio jets,the collimation mechanism and the role of magnetic field have been studied extensively by astronomers.In recent years,with the development of high-resolution VLBI observational techniques,radio astronomical observations have been able to probe the nuclear region of nearby AGN,which enables the study of the internal structure and physical processes of the jets.As a result,astronomers have made great progress in the observational study of jet collimation mechanisms in nearby radio galaxies.First,several mainstream jet production models are presented,followed by a review of the recent progress in the study of the collimation mechanism of FR-I and FR-II radio galaxies by presenting typical case studies.Finally,we make a summary and give a short prospect for the future study of jet collimation mechanism in radio galaxies.
Keyword射电星系 喷流 准直机制 甚长基线干涉测量
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Indexed ByCSCD ; 中文核心期刊要目总览
Language中文
CSCD IDCSCD:7261286
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5085
Collection射电天文研究室_星系宇宙学研究团组
Corresponding Author崔朗
Affiliation1.中国科学院 新疆天文台,乌鲁木齐 830011;
2.中国科学院 上海天文台,上海 200030
Recommended Citation
GB/T 7714
沈玉玲,崔朗,安涛,等. 射电星系喷流准直机制研究进展[J]. 天文学进展,2022,40(1):18-36.
APA 沈玉玲,崔朗,安涛,&刘祥.(2022).射电星系喷流准直机制研究进展.天文学进展,40(1),18-36.
MLA 沈玉玲,et al."射电星系喷流准直机制研究进展".天文学进展 40.1(2022):18-36.
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