The Astrophysical Journal Letters (Jan 2024)

NICER Discovery that SRGA J144459.2–604207 Is an Accreting Millisecond X-Ray Pulsar

  • Mason Ng,
  • Paul S. Ray,
  • Andrea Sanna,
  • Tod E. Strohmayer,
  • Alessandro Papitto,
  • Giulia Illiano,
  • Arianna C. Albayati,
  • Diego Altamirano,
  • Tuğba Boztepe,
  • Tolga Güver,
  • Deepto Chakrabarty,
  • Zaven Arzoumanian,
  • D. J. K. Buisson,
  • Elizabeth C. Ferrara,
  • Keith C. Gendreau,
  • Sebastien Guillot,
  • Jeremy Hare,
  • Gaurava K. Jaisawal,
  • Christian Malacaria,
  • Michael T. Wolff

DOI
https://doi.org/10.3847/2041-8213/ad4edb
Journal volume & issue
Vol. 968, no. 1
p. L7

Abstract

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We present the discovery, with the Neutron Star Interior Composition Explorer (NICER), that SRGA J144459.2−604207 is a 447.9 Hz accreting millisecond X-ray pulsar (AMXP), which underwent a 4 week long outburst starting on 2024 February 15. The AMXP resides in a 5.22 hr binary, orbiting a low-mass companion donor with M _d > 0.1 M _⊙ . We report on the temporal and spectral properties from NICER observations during the early days of the outburst, from 2024 February 21 through 2024 February 23, during which NICER also detected a type I X-ray burst that exhibited a plateau lasting ∼6 s. The spectra of the persistent emission were well described by an absorbed thermal blackbody and power-law model, with blackbody temperature kT ≈ 0.9 keV and power-law photon index Γ ≈ 1.9. Time-resolved burst spectroscopy confirmed the thermonuclear nature of the burst, where an additional blackbody component reached a maximum temperature of nearly kT ≈ 3 keV at the peak of the burst. We discuss the nature of the companion as well as the type I X-ray burst.

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