PASHAM, D. R., E. R. COUGHLIN, Michal ZAJAČEK, Itai LINIAL, Petra SUKOVÁ, C. J. NIXON, Agnieszka JANIUK, M. SNIEGOWSKA, Vojtěch WITZANY, Vladimír KARAS, M. KRUMPE, D. ALTAMIRANO, T. WEVERS and Riccardo ARCODIA. Alive but Barely Kicking: News from 3+ yr of Swift and XMM-Newton X-Ray Monitoring of Quasiperiodic Eruptions from eRO-QPE1. Astrophysical Journal Letters. IOP Publishing Ltd, 2024, vol. 963, No 2, p. 1-13. ISSN 2041-8205. Available from: https://dx.doi.org/10.3847/2041-8213/ad2a5c.
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Basic information
Original name Alive but Barely Kicking: News from 3+ yr of Swift and XMM-Newton X-Ray Monitoring of Quasiperiodic Eruptions from eRO-QPE1
Authors PASHAM, D. R., E. R. COUGHLIN, Michal ZAJAČEK (703 Slovakia, belonging to the institution), Itai LINIAL, Petra SUKOVÁ (203 Czech Republic), C. J. NIXON, Agnieszka JANIUK, M. SNIEGOWSKA, Vojtěch WITZANY, Vladimír KARAS (203 Czech Republic), M. KRUMPE, D. ALTAMIRANO, T. WEVERS and Riccardo ARCODIA.
Edition Astrophysical Journal Letters, IOP Publishing Ltd, 2024, 2041-8205.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW URL arXiv
Impact factor Impact factor: 7.900 in 2022
Organization unit Faculty of Science
Doi http://dx.doi.org/10.3847/2041-8213/ad2a5c
UT WoS 001181030400001
Keywords in English Tidal disruption; Black hole physics; High energy astrophysics; Supermassive black holes; Astronomy data analysis; X-ray astronomy; X-ray sources
Tags rivok
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 28/3/2024 09:58.
Abstract
Quasiperiodic eruptions (QPEs) represent a novel class of extragalactic X-ray transients that are known to repeat at roughly regular intervals of a few hours to days. Their underlying physical mechanism is a topic of heated debate, with most models proposing that they originate either from instabilities within the inner accretion flow or from orbiting objects. At present, our knowledge of how QPEs evolve over an extended timescale of multiple years is limited, except for the unique QPE source GSN 069. In this study, we present results from strategically designed Swift observing programs spanning the past 3 yr, aimed at tracking eruptions from eRO-QPE1. Our main results are as follows: (1) the recurrence time of eruptions can vary from flare to flare and is in the range of 0.6-1.2 days; (2) there is no detectable secular trend in evolution of the recurrence times; (3) consistent with prior studies, their eruption profiles can have complex shapes; and (4) the peak flux of the eruptions has been declining over the past 3 yr, with the eruptions barely detected in the most recent Swift data set taken in 2023 June. This trend of weakening eruptions has been reported recently in GSN 069. However, because the background luminosity of eRO-QPE1 is below our detection limit, we cannot verify whether the weakening is correlated with the background luminosity (as is claimed to be the case for GSN 069). We discuss these findings within the context of various proposed QPE models.
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GM24-10599M, research and development projectName: Hvězdy v galaktických jádrech: vzájemný vztah s masivními černými dírami
Investor: Czech Science Foundation, Stars in galactic nuclei: interrelation with massive black holes
90140, large research infrastructuresName: e-INFRA CZ
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