中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Optical intraday variability analysis for the BL Lacertae object 1ES 1426+42.8

文献类型:期刊论文

AuthorChang, X7; Xiong DR(熊定荣)6; Yi, T F4,5; Liu, C X7; Bhatta, G3; Xu, J R2; Gong, Y L1
SourceMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Issued Date2024-08-07
Volume533Issue:1Pages:120-130
Keywordgalaxies: active BL Lacertae objects: general BL Lacertae objects: individual (1ES 1426+42.8) galaxies: photometry
ISSN0035-8711
DOI10.1093/mnras/stae1839
Rank第2完成单位
SubtypeArticle
English AbstractThe observation data of blazar 1ES 1426+42.8 were obtained using the 1.02 m optical telescope of Yunnan Observatories during 2021 to 2023. Intraday variability (IDV) is detected on seven nights. We use the turbulent model to investigate the mechanism of IDV in 1ES 1426+42.8. The fitting light curves match the actual IDV curves well. Using this model, we obtain the parameters such as the size of turbulent cells and the width of pulses in the jet. A possible short-lived quasi-periodic oscillation (QPO) of 58.55 pm 8.09 min was detected on 2022 April 26 whose light curve exhibits eight cycles at 3 sigma global significance and confirmed by several different techniques. Through a more detailed analysis of the light curve of this night, we find that the period is shortened from 54.23 min (4 sigma) to 29.71 min (3 sigma). The possible QPO and period shortening phenomenon are best explained by the processes of magnetic reconnections.
Subject天文学 ; 星系与宇宙学
URL查看原文
Publish PlaceGREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
WOS KeywordQUASI-PERIODIC OSCILLATIONS ; ACTIVE GALACTIC NUCLEI ; GAMMA-RAY VARIABILITY ; BLAZAR S5 0716+714 ; MICROVARIABILITY PROPERTIES ; LIGHT-CURVE ; RADIO ; TIMESCALES ; PHOTOMETRY ; INSTABILITY
Funding ProjectNational Natural Science Foundation of China[11863007]; National Natural Science Foundation of China[12063005]; National Natural Science Foundation of China[12063007]; National Natural Science Foundation of China[11703078]; Yunnan Province Foundation[2019FB004]; Program for Innovative Research Team (in Science and Technology) in University of Yunnan Province (IRTSTYN); Yunnan Local Colleges Applied Basic Research Projects[2019FH001-12]; China Manned Space Project[CMS-CSST-2021-A06]; Science & Technology Champion Project[202005AB160002]; Yunnan Revitalization Talent Support Program[202105AE160021]; Yunnan Revitalization Talent Support Program[202305AT350002]; Program of the Polish Ministry of Science under the title 'Regional Excellence Initiative', project[RID/SP/0050/2024/1]
WOS Research AreaAstronomy & Astrophysics
Language英语
WOS IDWOS:001285375900003
PublisherOXFORD UNIV PRESS
Funding OrganizationNational Natural Science Foundation of China[11863007, 12063005, 12063007, 11703078] ; Yunnan Province Foundation[2019FB004] ; Program for Innovative Research Team (in Science and Technology) in University of Yunnan Province (IRTSTYN) ; Yunnan Local Colleges Applied Basic Research Projects[2019FH001-12] ; China Manned Space Project[CMS-CSST-2021-A06] ; Science & Technology Champion Project[202005AB160002] ; Yunnan Revitalization Talent Support Program[202105AE160021, 202305AT350002] ; Program of the Polish Ministry of Science under the title 'Regional Excellence Initiative', project[RID/SP/0050/2024/1]
Version出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27513]  
Collection云南天文台_丽江天文观测站(南方基地)
Affiliation1.Department of Astronomy, School of Physics and Astronomy, Yunnan University, Kunming 650091, People’s Republic of China
2.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai 264209, People’s Republic of China;
3.Janusz Gil Institute of Astronomy, University of Zielona Góra, ul. Szafrana 2, PL-65-516 Zielona Góra, Poland;
4.Guangxi Key Laboratory for the Relativistic Astrophysics, Nanning 530004, People’s Republic of China;
5.Key Laboratory of Colleges and Universities in Yunnan Province for High-energy Astrophysics, Department of Physics, Yunnan Normal University, Kunming 650500, People’s Republic of China;
6.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People’s Republic of China;
7.South-Western Institute for Astronomy Research, Yunnan University, Kunming 650500, People’s Republic of China;
Recommended Citation
GB/T 7714
Chang, X,Xiong DR,Yi, T F,et al. Optical intraday variability analysis for the BL Lacertae object 1ES 1426+42.8[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,533(1):120-130.
APA Chang, X.,熊定荣.,Yi, T F.,Liu, C X.,Bhatta, G.,...&Gong, Y L.(2024).Optical intraday variability analysis for the BL Lacertae object 1ES 1426+42.8.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,533(1),120-130.
MLA Chang, X,et al."Optical intraday variability analysis for the BL Lacertae object 1ES 1426+42.8".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 533.1(2024):120-130.

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来源:云南天文台

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