X-ray quasi-periodic eruptions from two previously quiescent galaxies

• Main Authors: Arcodia, R (Author), Merloni, A (Author), Nandra, K (Author), Buchner, J (Author), Salvato, M (Author), Pasham, D (Author), Remillard, R (Author), Comparat, J (Author), Lamer, G (Author), Ponti, G (Author), Malyali, A (Author), Wolf, J (Author), Arzoumanian, Z (Author), Bogensberger, D (Author), Buckley, DAH (Author), Gendreau, K (Author), Gromadzki, M (Author), Kara, E (Author), Krumpe, M (Author), Markwardt, C (Author), Ramos-Ceja, ME (Author), Rau, A (Author), Schramm, M (Author), Schwope, A (Author)
• Format: Article
• Language: English
• Published: Springer Science and Business Media LLC, 2022-04-20T16:41:31Z.
• Subjects: Article
• Online Access: Get fulltext

<jats:title>Abstract</jats:title><jats:p>Quasi-periodic eruptions (QPEs) are very-high-amplitude bursts of X-ray radiation recurring every few hours and originating near the central supermassive black holes of galactic nuclei<jats:sup>1,2</jats:sup>. It is currently unknown what triggers these events, how long they last and how they are connected to the physical properties of the inner accretion flows. Previously, only two such sources were known, found either serendipitously or in archival data<jats:sup>1,2</jats:sup>, with emission lines in their optical spectra classifying their nuclei as hosting an actively accreting supermassive black hole<jats:sup>3,4</jats:sup>. Here we report observations of QPEs in two further galaxies, obtained with a blind and systematic search of half of the X-ray sky. The optical spectra of these galaxies show no signature of black hole activity, indicating that a pre-existing accretion flow that is typical of active galactic nuclei is not required to trigger these events. Indeed, the periods, amplitudes and profiles of the QPEs reported here are inconsistent with current models that invoke radiation-pressure-driven instabilities in the accretion disk<jats:sup>5-9</jats:sup>. Instead, QPEs might be driven by an orbiting compact object. Furthermore, their observed properties require the mass of the secondary object to be much smaller than that of the main body<jats:sup>10</jats:sup>, and future X-ray observations may constrain possible changes in their period owing to orbital evolution. This model could make QPEs a viable candidate for the electromagnetic counterparts of so-called extreme-mass-ratio inspirals<jats:sup>11-13</jats:sup>, with considerable implications for multi-messenger astrophysics and cosmology<jats:sup>14,15</jats:sup>.</jats:p>