首页|A Possible X-ray Quasi-periodic Oscillation in the Narrow-line Seyfert 1 Galaxy Mrk 142

A Possible X-ray Quasi-periodic Oscillation in the Narrow-line Seyfert 1 Galaxy Mrk 142

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A possible quasi-periodic oscillation(QPO)at frequency 7.045 x 10-5 Hz is found in the narrow-line Seyfert 1 galaxy Mrk 142 in the data of XMM-Newton collected on 2020 April 11.We find that the QPO signal is statistically significantly larger than the 5σ level and highly coherent with quality factor Q>5 at the 0.3-10 keV band by using the method of the Lomb-Scargle Periodogram,the Weighted Wavelet Z-transform and the REDFIT.We analyze the data in 0.3-0.6keV,0.6-1 keV,1-3 keV and 3-10 keV energy bands,and find obvious QPO signals at 0.3-0.6 keV and 1-3 keV bands.We then analyze the time-average spectra and time variability at the QPO frequency of 7.045 x 10-5 Hz,and use a model to fit them.We find that the QPO signal mainly comes from the X-ray hot corona.

X-rays:galaxiesgalaxies:Seyfertaccretionaccretion disksradiation mechanisms:general

Xiao-Gu Zhong、Jian-Cheng Wang、Yong-Yun Chen、Xiao-Ling Yu

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College of Physics and Electronic Engineering,Qujing Normal University,Qujing 655011,China

Yunnan Observatories,Chinese Academy of Sciences,Kunming 650216,China

the Science Foundation of Department of Education of Yunnan Province

2024J0935

2024

天文和天体物理学研究
中国科学院国家天文台

天文和天体物理学研究

CSTPCD
影响因子:0.406
ISSN:1674-4527
年,卷(期):2024.24(6)