A new catalog of head–tail radio galaxies from LoTSS DR1

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Sabyasachi Pal, Shobha Kumari
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引用次数: 2

Abstract

The unique morphology of head–tail (HT) radio galaxies suggests that radio jets and their intra-cluster medium interact strongly. We conducted a systematic search for HT radio galaxies using the LOFAR two-meter sky survey first data release (LoTSS DR1) at 144 MHz. In this paper, a catalog of 55 new HT radio galaxies is presented, 10 of which are narrow-angle tailed sources (NATs) and 45 are wide-angle-tailed sources (WATs). NATs are characterized by tails that are bent like a narrow ‘V’ shape with a <90\(^{\circ }\) opening angle. The opening angle between jets in WAT radio galaxies is >90\(^{\circ }\), exhibiting wide ‘C’-like morphologies. We found that 30 out of 55 HT radio galaxies reported in this paper are associated with known galaxy clusters. Most of the sources presented in the current paper have redshifts <0.5. Various physical properties and statistical studies of these HT radio galaxies are presented.

来自LoTSS DR1的正尾射电星系新目录
正尾射电星系的独特形态表明射电喷流和它们的星系团内介质相互作用强烈。我们利用144 MHz的LOFAR两米巡天第一次数据发布(LoTSS DR1)对高温射电星系进行了系统的搜索。本文介绍了55个新的高温射电星系的星表,其中10个为窄角尾源,45个为广角尾源。NATs的特点是尾部弯曲成一个狭窄的“V”形,开口角为&lt;90 \(^{\circ }\)。WAT射电星系中喷流之间的开口角度为&gt;90 \(^{\circ }\),显示出宽的“C”状形态。我们发现,在这篇论文中报道的55个高温射电星系中,有30个与已知的星系团有关。本文中介绍的大多数源都有0.5的红移。介绍了这些高温射电星系的各种物理性质和统计研究。
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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来源期刊
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy 地学天文-天文与天体物理
CiteScore
1.80
自引率
9.10%
发文量
84
审稿时长
>12 weeks
期刊介绍: The journal publishes original research papers on all aspects of astrophysics and astronomy, including instrumentation, laboratory astrophysics, and cosmology. Critical reviews of topical fields are also published. Articles submitted as letters will be considered.
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