2023A&A...675A.152Q


Query : 2023A&A...675A.152Q

2023A&A...675A.152Q - Astronomy and Astrophysics, volume 675A152 (2023/7-1)

Tormund's return: Hints of quasi-periodic eruption features from a recent optical tidal disruption event.

QUINTIN E., WEBB N.A., GUILLOT S., MINIUTTI G., KAMMOUN E.S., GIUSTINI M., ARCODIA R., SOUCAIL G., CLERC N., AMATO R. and MARKWARDT C.B.

Abstract (from CDS):

Context. Quasi-periodic eruptions (QPEs) are repeating thermal X-ray bursts associated with accreting massive black holes, the precise underlying physical mechanisms of which are still unclear.
Aims. We present a new candidate QPE source, AT 2019vcb (nicknamed Tormund by the Zwicky Transient Facility Collaboration), which was found during an archival search for QPEs in the XMM-Newton archive. It was first discovered in 2019 as an optical tidal disruption event (TDE) at z = 0.088, and its X-ray follow-up exhibited QPE-like properties. Our goals are to verify its robustness as QPE candidate and to investigate its properties to improve our understanding of QPEs.
Methods. We performed a detailed study of the X-ray spectral behaviour of this source over the course of the XMM-Newton archival observation. We also report on recent Swift and NICER follow-up observations to constrain the source's current activity and overall lifetime, as well as an optical spectral follow-up.
Results. The first two Swift detections and the first half of the 30 ks XMM-Newton exposure of Tormund displayed a decaying thermal emission typical of an X-ray TDE. However, the second half of the exposure showed a dramatic rise in temperature (from $ 53.5^{+9.2}_{-7.7} $ eV to $ 113.8^{+2.9}_{-2.7} $ eV) and 0.2-2 keV luminosity (from $ 3.2^{+1.6}_{-1.0}\times10^{42} $ erg s–1 to $ 1.19^{+0.05}_{-0.05}\times10^{44} $ erg s–1) over ∼15 ks. The late-time NICER follow-up indicates that the source is still X-ray bright more than three years after the initial optical TDE.
Conclusions. Although only a rise phase was observed, Tormund's strong similarities with a known QPE source (eRO-QPE1) and the impossibility to simultaneously account for all observational features with alternative interpretations allow us to classify Tormund as a candidate QPE. If confirmed as a QPE, it would further strengthen the observational link between TDEs and QPEs. It is also the first QPE candidate for which an associated optical TDE was directly observed, constraining the formation time of QPEs.

Abstract Copyright: © The Authors 2023

Journal keyword(s): accretion, accretion disks - X-rays: general - quasars: supermassive black holes

Simbad objects: 11

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Number of rows : 11
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 OGLE16aaa ev 01 07 20.88 -64 16 20.7           ~ 72 0
2 2dFGRS TGS564Z081 Sy2 01 19 08.6635573080 -34 11 30.527946780   16.226   15.275   ~ 159 0
3 3C 50 Rad 01 44.4 +51 33           ~ 19 0
4 eRASSU J023147.2-102010 X 02 31 47.260 -10 20 10.31           ~ 72 0
5 eRASSU J023448.9-441931 X 02 34 48.970 -44 19 31.65           ~ 71 0
6 LEDA 1061293 AG? 02 49 17.3199268944 -04 12 52.076014416           ~ 65 0
7 HD 289002 * 06 45 13.3725491952 +02 08 14.685250596 10.06 10.62 10.44     B1 277 0
8 4XMM J123103.2+110648 X 12 31 03.233 +11 06 48.59           ~ 2 0
9 2XMM J123103.2+110648 AG? 12 31 03.239 +11 06 48.60           ~ 56 0
10 AT 2019vcb ev 12 38 56.38 +33 09 57.3           ~ 33 0
11 Z 160-104 SyG 13 02 00.1383745104 +27 46 57.854731080   15.4       ~ 159 0

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