Evidence for a Delayed UV Counterpart to X-ray Quasi-periodic Eruptions in Ansky
Hengxiao Guo, Zhen Yan, Ya-Ping Li, Joheen Chakraborty, Paula S\'anchez-S\'aez, Lorena Hern\'andez-Garc\'ia, Wenda Zhang, Jingbo Sun, Shuang-liang Li, Hongping Deng, Wenwen Zuo, Hiromichi Tagawa, Xin Pan, Minghao Zhang, Patricia Ar\'evalo, Paulina Lira, Chichuan Jin, Minfeng Gu

TL;DR
This paper reports the first detection of a UV response linked to X-ray quasi-periodic eruptions in the galaxy Ansky, revealing a delayed UV emission that provides new insights into the physical mechanisms of QPEs.
Contribution
It presents the first observation of a UV counterpart to X-ray QPEs, with a measured delay, in the galaxy Ansky, offering new constraints for QPE models.
Findings
UV emission lags X-ray eruptions by about 1 day.
UV response shows coherent periodic modulation over five cycles.
The delay may be due to diffusion or light-crossing time in the system.
Abstract
X-ray quasi-periodic eruptions (QPEs) represent a novel population of extreme, repeating nuclear transients whose physical origins remain debated. A defining characteristic of QPEs has been their exclusive detection in the X-ray band, with a notable absence of correlated multi-wavelength counterparts. Here we report the first detection of a recurrent UV response temporally coupled to the X-ray QPE signal in the source Ansky/ZTF19acnskyy. The UV emission displays coherent periodic modulations over five consecutive cycles, systematically lagging the X-ray eruptions by days, with a cross-correlation coefficient of . We suggest that the detectability of this corresponding signal may be enabled by Ansky's unusually long recurrence timescale, which could reduce the temporal smearing of the UV response seen in more rapid QPEs. The observed delay may…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Cosmic Phenomena · Crystallography and Radiation Phenomena
