2025ApJ...994L..16Z


Query : 2025ApJ...994L..16Z

2025ApJ...994L..16Z - Astrophys. J., 994, L16 (2025/November-3)

Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasiperiodic Eruptions.

ZHU J., JIANG N., WANG Y., WANG T., SUN L., ZHONG S., YAO Y., CHORNOCK R., DAI L., LYU J., SHU X., FREMLING C., HAMMERSTEIN E., HUANG S., LI W. and YOU B.

Abstract (from CDS):

X-ray quasiperiodic eruptions (QPEs) are rare and enigmatic phenomena that increasingly show a connection to tidal disruption events (TDEs). However, the recently discovered QPEs in ZTF19acnskyy (“Ansky”) appear to be linked to an active galactic nucleus (AGN) rather than a TDE, as their slow decay and AGN-like variability differ markedly from that of typical TDEs. This finding may imply broader formation channels for QPEs. To further investigate Ansky's nature, we obtained a timely ultraviolet (UV) spectrum, which reveals a featureless, TDE-like spectrum devoid of broad optical or UV emission lines. Additionally, the steep UV continuum, fitted by a power law with an index of -2.6, aligns more closely with TDEs than with AGNs. Compared to other featureless TDEs, Ansky exhibits a significantly lower blackbody luminosity (∼1043 erg s–1) and much longer rise/decay timescales, suggesting a distinct TDE subclass. An offset TDE involving an intermediate-mass black hole is unlikely, given its position consistent with the galactic center, with a 3σ upper limit of 54 pc. Instead, we propose that Ansky may result from the tidal disruption of a post-main-sequence star by a typical supermassive black hole. Our findings strengthen the growing evidence for TDE-QPE associations, although other formation channels for QPEs remain plausible and await future observational efforts.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Tidal disruption - Supermassive black holes - High energy astrophysics - Time domain astronomy

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 17

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Number of rows : 17
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 AT 2022upj ev 00 23 56.846 -14 25 23.22           ~ 30 0
2 2dFGRS TGS564Z081 Sy2 01 19 08.6635573080 -34 11 30.527946780   16.226   15.275   ~ 159 0
3 eRASSU J023147.2-102010 X 02 31 47.260 -10 20 10.31           ~ 72 0
4 eRASSU J023448.9-441931 X 02 34 48.970 -44 19 31.65           ~ 71 0
5 LEDA 1061293 AG? 02 49 17.3199268944 -04 12 52.076014416           ~ 65 0
6 AT 2021ehb ev 03 07 47.806 +40 18 40.57           ~ 42 0
7 NAME eRO-QPE5 G 03 25 43.2 -45 12 44           ~ 5 0
8 eRASSt J044534-101201 X 04 45 34.1 -10 12 00           ~ 25 0
9 AT 2019qiz ev 04 46 37.880 -10 13 34.92           ~ 143 0
10 AT 2022gri ev 07 18 20.778 +33 59 41.58           TDE 3 0
11 SDSS J090843.25+285229.8 QSO 09 08 43.2537866736 +28 52 29.798623560   19.03 18.83 18.55   ~ 32 0
12 EP 240222a ev 11 32 06.17 +27 00 17.6           ~ 6 0
13 AT 2019vcb ev 12 38 56.38 +33 09 57.3           ~ 33 0
14 Z 160-104 SyG 13 02 00.1383745104 +27 46 57.854731080   15.4       ~ 159 0
15 LEDA 3091738 G 13 35 19.9161300192 +07 28 07.533195564           ~ 19 0
16 1eRASS J140053.3-284558 X 14 00 53.3 -28 45 58           ~ 28 0
17 ASASSN -20hx SN? 17 03 36.541 +62 01 32.36           ~ 18 0

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