A radio flare associated with the nuclear transient eRASSt J234403-352640: an outflow launched by a potential tidal disruption event

被引:2
|
作者
Goodwin, A. J. [1 ]
Anderson, G. E. [1 ]
Miller-Jones, J. C. A. [1 ]
Malyali, A. [2 ]
Grotova, I [2 ]
Homan, D. [3 ]
Kawka, A. [1 ]
Krumpe, M. [3 ]
Liu, Z. [2 ]
Rau, A. [2 ]
机构
[1] Curtin Univ, Int Ctr Radio Astron Res, GPO Box U1987, Perth, WA 6845, Australia
[2] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
[3] Leibniz Inst Astrophys Potsdam, Sternwarte 16, 14482 Potsdam, Germany
基金
澳大利亚研究理事会;
关键词
radio continuum: transients; transients: tidal disruption events; keyword3; SYNCHROTRON SELF-ABSORPTION; X-RAY VARIABILITY; BLACK-HOLES; GALACTIC NUCLEI; EMISSION; OUTBURSTS; MODELS; AGN; MILLIMETER; GALAXIES;
D O I
10.1093/mnras/stae362
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an extensive radio monitoring campaign of the nuclear transient eRASSt J234402.9-352640 with the Australia Telescope Compact Array, one of the most X-ray luminous TDE candidates discovered by the SRG/eROSITA all-sky survey. The observations reveal a radio flare lasting >1000 d, coincident with the X-ray, UV, optical, and infrared flare of this transient event. Through modelling of the 10 epochs of radio spectral observations obtained, we find that the radio emission is well-described by an expanding synchrotron emitting region, consisting of a single ejection of material launched coincident with the optical flare. We conclude that the radio flare properties of eRASSt J234402.9-352640 are consistent with the population of radio-emitting outflows launched by non-relativistic tidal disruption events, and that the flare is likely due to an outflow launched by a tidal disruption event (but could also be a due to a new AGN accretion event) in a previously turned-off AGN.
引用
收藏
页码:7123 / 7136
页数:14
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