A possible γ-ray quasi-periodic oscillation of ∼314 days in the blazar OJ 287

被引:32
作者
Kushwaha, Pankaj [1 ,2 ]
Sarkar, Arkadipta [3 ]
Gupta, Alok C. [1 ]
Tripathi, Ashutosh [4 ,5 ]
Wiita, Paul J. [6 ]
机构
[1] Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263002, Nainital, India
[2] Univ Sao Paulo, Dept Astron IAG USP, BR-05508090 Sao Paulo, Brazil
[3] Tata Inst Fundamental Res, Dept High Energy Phys, Mumbai 400005, Maharashtra, India
[4] Fudan Univ, Ctr Field Theory & Particle Phys, 220 Handan Rd, Shanghai 200433, Peoples R China
[5] Fudan Univ, Dept Phys, 220 Handan Rd, Shanghai 200433, Peoples R China
[6] Coll New Jersey, Dept Phys, POB 7718, Ewing, NJ 08628 USA
基金
巴西圣保罗研究基金会;
关键词
radiation mechanisms: non-thermal; galaxies: active; galaxies: jets; quasars: individual: OJ 287; gamma-rays: galaxies; LIGHT CURVES; VARIABILITY; OJ-287; MULTIWAVELENGTH; NOISE;
D O I
10.1093/mnras/staa2899
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the detection of a probable gamma-ray quasi-periodic oscillation (QPO) of around 314 d in the monthly binned 0.1-300 GeV gamma-ray Fermi-Large Area Telescope light curve of the well-known BL Lacertae blazar OJ 287. To identify and quantify the QPO nature of the gamma-ray light curve of OJ 287, we used the Lomb-Scargle periodogram (LSP), REDFIT, and weighted wavelet Z-transform (WWZ) analyses. We briefly discuss possible emission models for radio-loud active galactic nuclei that can explain a gamma-ray QPO of such a period in a blazar.
引用
收藏
页码:653 / 658
页数:6
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