Optical intraday variability analysis for the BL Lacertae object 1ES 1426+42.8
文献类型:期刊论文
Author | Chang, X7; Xiong DR(熊定荣)6; Yi, T F4,5; Liu, C X7; Bhatta, G3; Xu, J R2; Gong, Y L1 |
Source | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
Issued Date | 2024-08-07 |
Volume | 533Issue:1Pages:120-130 |
Keyword | galaxies: active BL Lacertae objects: general BL Lacertae objects: individual (1ES 1426+42.8) galaxies: photometry |
ISSN | 0035-8711 |
DOI | 10.1093/mnras/stae1839 |
Rank | 第2完成单位 |
Subtype | Article |
English Abstract | The 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 Place | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
WOS Keyword | QUASI-PERIODIC OSCILLATIONS ; ACTIVE GALACTIC NUCLEI ; GAMMA-RAY VARIABILITY ; BLAZAR S5 0716+714 ; MICROVARIABILITY PROPERTIES ; LIGHT-CURVE ; RADIO ; TIMESCALES ; PHOTOMETRY ; INSTABILITY |
Funding Project | National 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 Area | Astronomy & Astrophysics |
Language | 英语 |
WOS ID | WOS:001285375900003 |
Publisher | OXFORD UNIV PRESS |
Funding Organization | National 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) |
Affiliation | 1.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. |
入库方式: OAI收割
来源:云南天文台
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