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The radio detection and accretion properties of the peculiar nuclear transient AT 2019avd

Wang, Yanan (author)
University of Southampton
Baldi, Ranieri D. (author)
University of Southampton,Istituto nazionale di astrofisica (INAF)
Del Palacio, Santiago, 1990 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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Guolo, Muryel (author)
Johns Hopkins University
Yang, Xiaolong (author)
Chinese Academy of Sciences
Zhang, Yangkang (author)
Chinese Academy of Sciences
Done, Chris (author)
Durham University
Pasham, Dheeraj R. (author)
Massachusetts Institute of Technology (MIT)
Qiao, Erlin (author)
Chinese Academy of Sciences
Jiang, Ning (author)
University of Science and Technology of China
Yan, Hongliang (author)
Chinese Academy of Sciences
Panessa, Francesca (author)
Istituto nazionale di astrofisica (INAF)
Jin, Chichuan (author)
Chinese Academy of Sciences
Shen, Rongfeng (author)
Sun Yat-Sen University
Dai, Lixin (author)
The University of Hong Kong
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 (creator_code:org_t)
2023-01-11
2023
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 520:2, s. 2417-2435
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • AT 2019avd is a nuclear transient detected from infrared to soft X-rays, though its nature is yet unclear. The source has shown two consecutive flaring episodes in the optical and the infrared bands, and its second flare was covered by X-ray monitoring programs. During this flare, the UVOT/Swift photometries revealed two plateaus: one observed after the peak and the other one appeared similar to 240 d later. Meanwhile, our NICER and XRT/Swift campaigns show two declines in the X-ray emission, one during the first optical plateau and one 70-90 d after the optical/UV decline. The evidence suggests that the optical/UV could not have been primarily originated from X-ray reprocessing. Furthermore, we detected a timelag of similar to 16-34 d between the optical and UV emission, which indicates the optical likely comes from UV reprocessing by a gas at a distance of 0.01-0.03 pc. We also report the first VLA and VLBA detection of this source at different frequencies and different stages of the second flare. The information obtained in the radio band - namely a steep and a late-time inverted radio spectrum, a high brightness temperature and a radio-loud state at late times - together with the multiwavelength properties of AT 2019avd suggests the launching and evolution of outflows such as disc winds or jets. In conclusion, we propose that after the ignition of black hole activity in the first flare, a super-Eddington flaring accretion disc formed and settled to a sub-Eddington state by the end of the second flare, associated with a compact radio outflow.

Subject headings

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Annan fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Other Physics Topics (hsv//eng)

Keyword

accretion discs
black hole physics
galaxies: nuclei
radio continuum: transients
accretion
galaxies: active

Publication and Content Type

art (subject category)
ref (subject category)

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