Spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498−2921 during its 2023 outburst

We present a comprehensive study of the spectral properties of the accreting millisecond X-ray pulsar IGR J17498−2921 during its 2023 outburst. Similar to other accreting millisecond X-ray pulsars, the broadband spectral emission observed quasi-simultaneously by NICER and NuSTAR is well described by an absorbed Comptonized emission with an electron temperature of ∼17 keV plus a disk reflection component. The broadening of the disk reflection spectral features, such as a prominent iron emission line at 6.4–6.7 keV, is consistent with the relativistic motion of matter in a disk truncated at ∼21 R g from the source, near the Keplerian corotation radius. From the high-cadence monitoring data obtained with NICER, we observed that the evolution of the photon index and the temperature of seed photons tracks variations in the X-ray flux. This is particularly evident close to a sudden ∼–0.25 cycle jump in the pulse phase, which occurs immediately following an X-ray flux flare and a drop in the pulse amplitude below the 3 σ detection threshold. We also report on the non-detection of optical pulsations with TNG/SiFAP2 from the highly absorbed optical counterpart.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-10-07
DOI
https://doi.org/10.1051/0004-6361/202451703
Citations
3
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.99

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article

Spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498−2921 during its 2023 outburst

F. Leone, A. Ghedina, A. Marino, Riccardo La Placa et al.
3 citations
Astronomy and Astrophysics
Astrophysical Phenomena and Observations
0.99
article

Spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498−2921 during its 2023 outburst

F. Leone, A. Ghedina, A. Marino, Riccardo La Placa, A. Papitto, T. Di Salvo, A. Sanna, F. Coti Zelati, M. Cecconi, G. Illiano, A. Miraval Zanon, Tod E. Strohmayer, C. Malacaria, Filippo Ambrosino, Caterina Ballocco, M. Gonzales
article en
3 citations

Abstract

We present a comprehensive study of the spectral properties of the accreting millisecond X-ray pulsar IGR J17498−2921 during its 2023 outburst. Similar to other accreting millisecond X-ray pulsars, the broadband spectral emission observed quasi-simultaneously by NICER and NuSTAR is well described by an absorbed Comptonized emission with an electron temperature of ∼17 keV plus a disk reflection component. The broadening of the disk reflection spectral features, such as a prominent iron emission line at 6.4–6.7 keV, is consistent with the relativistic motion of matter in a disk truncated at ∼21 R g from the source, near the Keplerian corotation radius. From the high-cadence monitoring data obtained with NICER, we observed that the evolution of the photon index and the temperature of seed photons tracks variations in the X-ray flux. This is particularly evident close to a sudden ∼–0.25 cycle jump in the pulse phase, which occurs immediately following an X-ray flux flare and a drop in the pulse amplitude below the 3 σ detection threshold. We also report on the non-detection of optical pulsations with TNG/SiFAP2 from the highly absorbed optical counterpart.

Astronomy and AstrophysicsVol. 691
University of Rome Tor Vergata (IT), Goddard Space Flight Center (US), Institute of Space Sciences (ES), University of Cagliari (IT), Astronomical Observatory of Rome (IT), Brera Astronomical Observatory (IT), Institut d'Estudis Espacials de Catalunya (ES), Joint Space Science Institute (US), Osservatorio Astrofisico di Catania (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari (IT), Telescopio Nazionale Galileo (ES), Deleted Institution, Sapienza University of Rome (IT), University of Palermo (IT)
National Aeronautics and Space Administration, California Institute of Technology, European Commission, Istituto Nazionale di Astrofisica, Jet Propulsion Laboratory
Openalex Percentile: Top 23%
Astrophysical Phenomena and Observations
0.99
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