Alive and Strongly Kicking: Stable X-ray Quasi-Periodic Eruptions from eRO-QPE2 over 3.5 Years
Dheeraj Pasham, Shubham Kejriwal, Eric Coughlin, Vojt\v{e}ch Witzany,, Alvin J. K. Chua, Michal Zaja\v{c}ek, Thomas Wevers, Yukta Ajay

TL;DR
This study presents a 3.5-year analysis of the stable and recurring X-ray eruptions from eRO-QPE2, providing insights into their consistency and implications for models like extreme mass ratio inspirals.
Contribution
The paper offers the first long-term detailed observational analysis of eRO-QPE2, highlighting its remarkable stability compared to other QPEs and discussing implications for theoretical models.
Findings
eRO-QPE2's eruption properties are remarkably stable over 3.5 years.
The recurrence time of eruptions is consistently around 2.35 hours.
Compared to other QPEs, eRO-QPE2 shows greater stability and more cycles over the same period.
Abstract
Quasi-periodic eruptions (QPEs) are recurring bursts of soft X-rays from the nuclei of galaxies. Their physical origin is currently a subject of debate, with models typically invoking an orbiter around a massive black hole or disk instabilities. Here we present and analyze the temporal and spectral evolution of the QPE source eRO-QPE2 over 3.5 years. We find that eRO-QPE2 1) is remarkably stable over the entire 3.5-year temporal baseline in its eruption peak luminosity, eruption temperature, quiescent temperature, and quiescent luminosity, 2) has a stable mean eruption recurrence time of 2.35 hours, with marginal (2) evidence for a hour reduction over the 3.5 yr period, and 3) has a long-short variation in its recurrence time in August 2020, but this pattern is absent from all subsequent observations. The stability of its peak eruption luminosity and that of the…
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Taxonomy
TopicsMedical Imaging Techniques and Applications · Nuclear Physics and Applications
