NuSTAR and NICER reveal IGR J17591–2342 as a new accreting millisecond X-ray pulsar
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Author(s)
Sanna, A.
Ferrigno, C.
Ray, P. S.
Ducci, L.
Jaisawal, G. K.
Enoto, T.
Bozzo, E.
Altamirano, D.
Di Salvo, T.
Strohmayer, T. E.
Date Issued
September 2018
Journal
Astronomy & Astrophysics
Publisher
EDP Sciences
Citation
Sanna, A., C. Ferrigno, P. S. Ray, L. Ducci, G. K. Jaisawal, T. Enoto, E. Bozzo, et al. “NuSTAR and NICER Reveal IGR J17591–2342 as a New Accreting Millisecond X-Ray Pulsar.” Astronomy & Astrophysics 617 (September 2018): L8. © 2018 ESO 2018
Version
Original manuscript
Abstract
We report the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER) of the accreting millisecond X-ray pulsar IGR J17591-2342. Coherent X-ray pulsations around 527.4 Hz (1.9 ms) with a clear Doppler modulation were detected. This implies an orbital period of ∼8.8 h and a projected semi-major axis of ∼1.23 lt-s. With the binary mass function, we estimate a minimum companion mass of 0.42 M, obtained assuming a neutron star mass of 1.4[subscript ⊙] and an inclination angle lower than 60°, as suggested by the absence of eclipses or dips in the light curve of the source. The broad-band energy spectrum, obtained by combining NuSTAR, swift and INTEGRAL observations, is dominated by Comptonisation of soft thermal seed photons with a temperature of ∼0.7 keV by electrons heated to 21 keV. We also detect black-body-like thermal direct emission that is compatible with an emission region of a few kilometers and a temperature compatible with the seed source of Comptonisation. A weak Gaussian line centred on the iron Kα complex can be interpreted as a signature of disc reflection. A similar spectrum characterises the NICER spectra, which was measured when the outburst faded. Key words: accretion, accretion disks / stars: low-mass / pulsars: general / stars: neutron / X-rays: binaries
MIT Department
Massachusetts Institute of Technology. Department of Physics
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DOI of Published Version
https://doi.org/10.1051/0004-6361/201834160
