The Astrophysical Journal (Jan 2023)

Identification of 1RXS J165424.6-433758 as a Polar Cataclysmic Variable

  • B. O’Connor,
  • J. Brink,
  • D. A. H. Buckley,
  • K. Mukai,
  • C. Kouveliotou,
  • E. Göğüş,
  • S. B. Potter,
  • P. Woudt,
  • A. Lien,
  • A. Levan,
  • O. Kargaltsev,
  • M. G. Baring,
  • E. Bellm,
  • S. B. Cenko,
  • P. A. Evans,
  • J. Granot,
  • C. Hailey,
  • F. Harrison,
  • D. Hartmann,
  • A. J. van der Horst,
  • D. Huppenkothen,
  • L. Kaper,
  • J. A. Kennea,
  • P. O. Slane,
  • D. Stern,
  • E. Troja,
  • R. A. M. J. Wijers,
  • G. Younes

DOI
https://doi.org/10.3847/1538-4357/acf831
Journal volume & issue
Vol. 957, no. 2
p. 89

Abstract

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We present the results of our X-ray, ultraviolet, and optical follow-up campaigns of 1RXS J165424.6-433758, an X-ray source detected with the Swift Deep Galactic Plane Survey. The source X-ray spectrum (Swift and NuSTAR) is described by thermal bremsstrahlung radiation with a temperature of kT = 10.1 ± 1.2 keV, yielding an X-ray (0.3–10 keV8) luminosity L _X = (6.5 ± 0.8) × 10 ^31 erg s ^−1 at a Gaia distance of 460 pc. Spectroscopy with the Southern African Large Telescope revealed a flat continuum dominated by emission features, demonstrating an inverse Balmer decrement, the λ 4640 Bowen blend, almost a dozen He i lines, and He ii λ 4541, λ 4686, and λ 5411. Our high-speed photometry demonstrates a preponderance of flickering and flaring episodes, and revealed the orbital period of the system, P _orb = 2.87 hr, which fell well within the cataclysmic variable (CV) period gap between 2 and 3 hr. These features classify 1RXS J165424.6-433758 as a nearby polar magnetic CV.

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