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Intermediate-mass black holes: finding of episodic, large-scale, and powerful jet activity in a dwarf galaxy
Yang, Jun1; Paragi, Zsolt2; Frey, Sándor3,4,5; Gurvits, Leonid I2,6; Liao, Mai7,8; Liu, Xiang9; Cui, Lang9; Yang, Xiaolong10; Chen W(陈文)1,11,12; Varenius, Eskil1; Conway, John E1; Chen, Rurong13,14; Chang, Ning9
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023-02-22
卷号520期号:4页码:5964-5973
DOI10.1093/mnras/stad493
产权排序第11完成单位
收录类别SCI ; EI
关键词galaxies:active galaxies:dwarf individual galaxies:individual:SDSS J090613.77+561015.2 radio continuum:galaxies
摘要Dwarf galaxies are characterized by a very low luminosity and low mass. Because of significant accretion and ejection activity of massive black holes, some dwarf galaxies also host lo w-luminosity acti ve galactic nuclei (AGNs). In a few dwarf AGNs, very long baseline interferometry (VLBI) observations have found faint non-thermal radio emission. SDSS J090613.77 + 561015.2 is a dwarf AGN owning an intermediate-mass black hole (IMBH) with a mass of M-BH = 3 . 6 (+5.9) (-2.3 )x 10 (5) M(? )and showing a rarely seen two-component radio structure in its radio nucleus. To further probe their nature, i.e. the IMBH jet activity, we performed additional deep observations with the European VLBI Network (EVN) at 1.66 and 4.99 GHz. We find the more diffuse emission regions and structure details. These new EVN imaging results allow us to reveal a two-sided jet morphology with a size up to about 150 mas (projected length similar to 140 pc) and a radio luminosity of about 3 x 10( 38) erg s( -1). The peak feature has an optically thin radio spectrum and thus more likely represents a relatively young ejecta instead of a jet base. The EVN study on SDSS J090613.77 + 561015.2 demonstrates the existence of episodic, relatively large-scale, and powerful IMBH jet activity in dwarf AGNs. Moreo v er, we collected a small sample of VLBI-detected dwarf AGNs and investigated their connections with normal AGNs. We notice that these radio sources in the dwarf AGNs tend to have steep spectra and small linear sizes, and possibly represent ejecta from scaled-down episodic jet activity.
资助项目EVN project[EY035] ; National SKA Program of China[2022SKA0120102] ; CAS `Light of West China' Program[2021-XBQNXZ-005] ; National Natural Science Foundation of China (NSFC)[U2031212] ; National Natural Science Foundation of China (NSFC)[61931002] ; Hungarian National Research, Development and Innovation Office[OTKA K134213] ; NSFC[11903079] ; NSFC[12103076] ; Shanghai Sailing Program[21YF1455300] ; China Postdoctoral Science Foundation[2021M693267]
项目资助者EVN project[EY035] ; National SKA Program of China[2022SKA0120102] ; CAS `Light of West China' Program[2021-XBQNXZ-005] ; National Natural Science Foundation of China (NSFC)[U2031212, 61931002] ; Hungarian National Research, Development and Innovation Office[OTKA K134213] ; NSFC[11903079, 12103076] ; Shanghai Sailing Program[21YF1455300] ; China Postdoctoral Science Foundation[2021M693267]
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
学科门类理学 ; 理学::天文学
文章类型Article
出版者OXFORD UNIV PRESS
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
WOS记录号WOS:000943248300020
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]COMPACT STEEP-SPECTRUM ; RADIO-SOURCE COUNTERPARTS ; GALACTIC NUCLEI ; VLBI OBSERVATIONS ; STAR-FORMATION ; X-RAY ; FUNDAMENTAL PLANE ; SNAPSHOT SURVEY ; CENTRAL ENGINE ; AGN
EI入藏号20232014101792
EI主题词Active Galactic Nuclei
EI分类号657.2 Extraterrestrial Physics and Stellar Phenomena - 716.3 Radio Systems and Equipment - 931.5 Gravitation, Relativity and String Theory
引用统计
被引频次:3[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/25878
专题射电天文研究组
通讯作者Yang, Jun
作者单位1.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, Sweden;
2.Joint Institute for VLBI ERIC, Oude Hoogevceensedijk 4, NL-7991 PD Dwingeloo, the Netherlands;
3.Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary;
4.CSFK, MTA Centre of Excellence, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary;
5.Institute of Physics, ELTE Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary;
6.Faculty of Aerospace Engineering, Delft University of Technology, Kluyverweg 1, NL-2629 HS Delft, the Netherlands;
7.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, Anhui 230026, China;
8.School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China;
9.Xinjiang Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi 830011, China;
10.Shanghai Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Shanghai 200030, China;
11.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650216, China;
12.University of Chinese Academy of Sciences, No. 19(A) Yuquan Road, Shijingshan District, Beijing 100049, China;
13.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;
14.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China
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Yang, Jun,Paragi, Zsolt,Frey, Sándor,et al. Intermediate-mass black holes: finding of episodic, large-scale, and powerful jet activity in a dwarf galaxy[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,520(4):5964-5973.
APA Yang, Jun.,Paragi, Zsolt.,Frey, Sándor.,Gurvits, Leonid I.,Liao, Mai.,...&Chang, Ning.(2023).Intermediate-mass black holes: finding of episodic, large-scale, and powerful jet activity in a dwarf galaxy.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,520(4),5964-5973.
MLA Yang, Jun,et al."Intermediate-mass black holes: finding of episodic, large-scale, and powerful jet activity in a dwarf galaxy".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 520.4(2023):5964-5973.
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