Exploring the connection between compact object mergers and fast X-ray transients

Context. The connection between compact object mergers and some extragalactic fast X-ray transients (FXRTs) has long been hypothesised but never ultimately established. Aims. In this work, we investigate two FXRTs, the LEIA X-ray Transient LXT 240402A and the Einstein Probe EP 250207b, whose precise positions lie close to nearby ( z ≲ 0.1) quiescent galaxies with a negligible probability of chance coincidence, identifying them as particularly promising cases of merger-driven explosions in the local Universe. Methods. We used Chandra to derive accurate localisations for both events and secure otherwise ambiguous associations with their optical counterparts. Deep optical and near-infrared observations with VLT, GTC, and LBT were performed to characterise the surrounding environment and search for kilonova emission, the hallmark of neutron star mergers. Complementary early-time X-ray monitoring with Swift and Einstein Probe was used to constrain the non-thermal afterglow. Results. We find that both FXRTs remain compatible with a compact binary merger progenitor, which produced low-mass ejecta and kilonova emission subdominant to the afterglow. However, alternative explanations such as a distant ( z ≳ 1) core-collapse supernova cannot be conclusively ruled out.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-12-08
DOI
https://doi.org/10.1051/0004-6361/202557612
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
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article

Exploring the connection between compact object mergers and fast X-ray transients

Richard S. Woolf, Hu Lei, Maria Gritsevich, A. Tsvetkova et al.
Astronomy and Astrophysics
Gamma-ray bursts and supernovae
article

Exploring the connection between compact object mergers and fast X-ray transients

Richard S. Woolf, Hu Lei, Maria Gritsevich, A. Tsvetkova, E. Troja, Qinyu Wu, Chris L. Fryer, J. E. Grove, A. Ridnaia, Melissa Kerr, R. L. Becerra, D. Frederiks, Hui Sun, Brendan O’Connor, H. W. Lee, D. Svinkin, S. Dichiara, Roberto Ricci, C. C. Cheung, A. J. Castro‐Tirado, Margarita Pereyra, R. Sánchez-Ramírez, Camila Angulo-Valdez, Yu-Han Yang, Mikhail Ulanov, M. G. Watson, Muskan Yadav, Bing Zhang, Massine El Kabir, Niccolò Passaleva, D. María Caballero-García, L. Alexandra Lysenko
article en

Abstract

Context. The connection between compact object mergers and some extragalactic fast X-ray transients (FXRTs) has long been hypothesised but never ultimately established. Aims. In this work, we investigate two FXRTs, the LEIA X-ray Transient LXT 240402A and the Einstein Probe EP 250207b, whose precise positions lie close to nearby ( z ≲ 0.1) quiescent galaxies with a negligible probability of chance coincidence, identifying them as particularly promising cases of merger-driven explosions in the local Universe. Methods. We used Chandra to derive accurate localisations for both events and secure otherwise ambiguous associations with their optical counterparts. Deep optical and near-infrared observations with VLT, GTC, and LBT were performed to characterise the surrounding environment and search for kilonova emission, the hallmark of neutron star mergers. Complementary early-time X-ray monitoring with Swift and Einstein Probe was used to constrain the non-thermal afterglow. Results. We find that both FXRTs remain compatible with a compact binary merger progenitor, which produced low-mass ejecta and kilonova emission subdominant to the afterglow. However, alternative explanations such as a distant ( z ≳ 1) core-collapse supernova cannot be conclusively ruled out.

Astronomy and AstrophysicsVol. 705
University of Rome Tor Vergata (IT), United States Naval Research Laboratory (US), Pennsylvania State University (US), Ural Federal University (RU), University of Helsinki (FI), University of Nevada, Reno (US), Los Alamos National Laboratory (US), University of Cagliari (IT), Chinese Academy of Sciences (CN), Astronomy and Space (AU), Instituto de Astrofísica de Andalucía (ES), National Astronomical Observatories (CN), Carnegie Mellon University (US), Universidad de Málaga (ES), Sapienza University of Rome (IT), University of Hong Kong (HK), Universidad Nacional Autónoma de México (MX), Netherlands Institute for Radio Astronomy (NL), Ioffe Institute (RU)
Openalex Percentile: Top 73%
Gamma-ray bursts and supernovae
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