Discovery of 105 Hz coherent pulsations in the ultracompact binary IGR J16597-3704

Authors
  • A. Sanna
  • A. Bahramian
  • E. Bozzo
  • C. Heinke
Publication date 14-02-2018
Journal Astronomy & Astrophysics
Article number L2
Volume | Issue number 610
Number of pages 4
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
We report the discovery of X-ray pulsations at 105.2 Hz (9.5 ms) from the transient X-ray binary IGR J16597–3704 using NuSTAR and Swift. The source was discovered by INTEGRAL in the globular cluster NGC 6256 at a distance of 9.1 kpc. The X-ray pulsations show a clear Doppler modulation that implies an orbital period of ~46 min and a projected semi-major axis of ~5 lt-ms, which makes IGR J16597–3704 an ultracompact X-ray binary system. We estimated a minimum companion mass of 6.5 × 10−10 M⊙, assuming a neutron star mass of 1.4 M⊙, and an inclination angle of <75° (suggested by the absence of eclipses or dips in its light curve). The broad-band energy spectrum of the source is well described by a disk blackbody component (kT ~ 1.4 keV) plus a comptonised power-law with photon index ~2.3 and an electron temperature of ~30 keV. Radio pulsations from the source were unsuccessfully searched for with the Parkes Observatory.
Document type Article
Language English
Published at https://doi.org/10.1051/0004-6361/201732262
Other links http://adsabs.harvard.edu/abs/2018A%26A...610L...2S
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