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

被引:0
|
作者
Illiano, G. [1 ,2 ,3 ]
Papitto, A. [1 ]
Marino, A. [4 ,5 ]
Strohmayer, T. E. [6 ,7 ]
Sanna, A. [8 ]
Di Salvo, T. [9 ]
La Placa, R. [1 ]
Ambrosino, F. [1 ]
Zanon, A. Miraval [10 ]
Zelati, F. Coti [4 ,5 ,11 ]
Ballocco, C. [1 ,3 ]
Malacaria, C. [1 ]
Ghedina, A. [12 ]
Cecconi, M. [12 ]
Gonzales, M. [12 ]
Leone, F. [13 ,14 ]
机构
[1] INAF Osservatorio Astron Roma, Via Frascati 33, I-00076 Monte Porzio Catone, RM, Italy
[2] Tor Vergata Univ Rome, Via Ric Sci 1, I-00133 Rome, Italy
[3] Sapienza Univ Roma, Piazzale Aldo Moro 5, I-00185 Rome, Italy
[4] CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain
[5] Inst Estudis Espacials Catalunya IEEC, E-08860 Castelldefels, Barcelona, Spain
[6] NASA Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA
[7] NASA Goddard Space Flight Ctr, Joint Space Sci Inst, Greenbelt, MD 20771 USA
[8] Univ Cagliari, Dipartimento Fis, SP Monserrato Sestu Km 0-7, I-09042 Monserrato, Italy
[9] Univ Palermo, Dipartimento Fis & Chim, Via Archirafi 36, I-90123 Palermo, Italy
[10] ASI Agenzia Spaziale Italiana, Via Politecn Snc, I-00133 Rome, Italy
[11] INAF Osservatorio Astron Brera, Via Bianchi 46, I-23807 Merate, LC, Italy
[12] Fdn Galileo Galilei INAF, La Palma, Spain
[13] Univ Catania, Dipartimento Fis & Astron, Sez Astrofis, Via S Sofia 78, I-95123 Catania, Italy
[14] INAF Osservatorio Astrofis Catania, Via S Sofia 78, I-95123 Catania, Italy
基金
欧洲研究理事会;
关键词
accretion; accretion disks; stars: neutron; pulsars: individual: IGR J17498-2921; X-rays: binaries; SAX J1808.4-3658; BROAD-BAND; XMM-NEWTON; SRGA J144459.2-604207; MAGNETIC-FIELDS; HOT-SPOTS; SPIN-DOWN; REFLECTION; DISCOVERY; SPECTROSCOPY;
D O I
10.1051/0004-6361/202451703
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 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 similar to 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 similar to-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 sigma 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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页数:14
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