中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Discovery of a Years-delayed Radio Flare from an Unusually Slowly Evolving Tidal Disruption Event Candidate

文献类型:期刊论文

作者Zhang, Zhumao8; Shu, Xinwen8; Yang, Lei8; Sun, Luming8; Ding, Hucheng8; Yan, Lin7; Jiang, Ning13; An, Fangxia6,9; Silima, Walter5; Zhang, Fabao8
刊名ASTROPHYSICAL JOURNAL
出版日期2026-01-20
卷号997期号:1
ISSN号0004-637X
DOI10.3847/1538-4357/ae29f0
产权排序第10完成单位
文献子类Article
英文摘要SDSS J1115+0544 is a unique low-ionization nuclear emission-line region galaxy with energetic ultraviolet (UV), optical, and mid-infrared outbursts occurring in its nucleus. We present the results from an analysis of multiwavelength photometric and radio follow-up observations with a time span of approximate to 9 yr since its discovery. We find that following a luminosity plateau of approximate to 500 days, the UV/optical emission has decayed back to the preoutburst level, suggesting that the nuclear outburst might be caused by a stellar tidal disruption event (TDE). In this case, J1115+0544 could be an unusually slowly evolving optical TDE with longest rise and decline time scales ever found. Three years later than the optical peak, a delayed radio brightening was found with a luminosity as high as nu L nu(5.5 GHz) similar to 1.9 x 1039 erg s-1. Using a standard equipartition analysis, we find that the outflow powering the radio emission was launched at t greater than or similar to 1150 days with a velocity of v less than or similar to 0.1c and a minimal kinetic energy of EK greater than or similar to 3 x 1049 erg. The delayed radio brightening coupled with the disappearing plateau in the UV/optical light curves is consistent with the scenario involving delayed ejection of an outflow from a state transition in the disk. SDSS J1115+0544 is the first TDE candidate displaying both a short-lived UV/optical plateau emission and a late-time radio brightening. Future radio observations of these TDEs in the postplateau decay phase will help to establish the connection between outflow launching and changes in accretion rate.
学科主题天文学 ; 星系与宇宙学
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词RAPID TURN-ON ; RELATIVISTIC OUTFLOW ; LUMINOSITY FUNCTION ; NEARBY GALAXIES ; JET ENERGETICS ; DISC FORMATION ; BLACK-HOLES ; ACCRETION ; EMISSION ; ASTROPY
资助项目MOST divided by National Natural Science Foundation of China (NSFC)[12192221]; Anhui Normal University (ANU)[2022SKA0130102]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001659790200001
出版者IOP Publishing Ltd
资助机构MOST divided by National Natural Science Foundation of China (NSFC)[12192221] ; Anhui Normal University (ANU)[2022SKA0130102]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28854]  
专题云南天文台_丽江天文观测站(南方基地)
通讯作者Shu, Xinwen
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People’s Republic of China;
2.Department of Astronomy, Guangzhou University, Guangzhou 510006, People’s Republic of China;
3.College of Physics, Guizhou University, Guiyang 550025, People’s Republic of China;
4.Indian Institute of Astrophysics (IIA), 2nd Block, Koramangala, Bengaluru, 560034, Karnataka, India;
5.Inter-University Institute for Data Intensive Astronomy (IDIA), Department of Astronomy, University of Cape Town, 7701 Rondebosch, Cape Town, South Africa;
6.Inter-University Institute for Data Intensive Astronomy (IDIA), Department of Physics and Astronomy, University of the Western Cape, 7535 Bellville, Cape Town, South Africa;
7.Caltech Optical Observatories, California Institute of Technology, Pasadena, CA 91125, USA;
8.Department of Physics, Anhui Normal University, Wuhu, Anhui 241002, People’s Republic of China; xwshu@ahnu.edu.cn;
9.Purple Mountain Observatory, Chinese Academy of Sciences, 10 Yuan Hua Road, Qixia District, Nanjing 210023, People’s Republic of China;
10.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China
推荐引用方式
GB/T 7714
Zhang, Zhumao,Shu, Xinwen,Yang, Lei,et al. Discovery of a Years-delayed Radio Flare from an Unusually Slowly Evolving Tidal Disruption Event Candidate[J]. ASTROPHYSICAL JOURNAL,2026,997(1).
APA Zhang, Zhumao.,Shu, Xinwen.,Yang, Lei.,Sun, Luming.,Ding, Hucheng.,...&Wang, Tinggui.(2026).Discovery of a Years-delayed Radio Flare from an Unusually Slowly Evolving Tidal Disruption Event Candidate.ASTROPHYSICAL JOURNAL,997(1).
MLA Zhang, Zhumao,et al."Discovery of a Years-delayed Radio Flare from an Unusually Slowly Evolving Tidal Disruption Event Candidate".ASTROPHYSICAL JOURNAL 997.1(2026).

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