HST spectrum and timing of the ultracompact X-ray binary candidate 47 Tuc X9

2018/02/01 by V. Tudor, Vlad Tudor, J. C. A. Miller‐Jones +29
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Binary number #Physics #Spectrum (functional analysis) #Stellar, planetary, and galactic studies #astro-ph.HE #astro-ph.SR

paper · pdf · doi:10.1093/mnras/sty284

20 pages, 12 figures. Accepted for publication in MNRAS

arxiv created 2018/02/01 · openalex publication_date 2018/02/02 · arxiv updated 2018/02/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

To confirm the nature of the donor star in the ultracompact X-ray binary candidate 47 Tuc X9, we obtained optical spectra (3000–10 000 Å) with the Hubble Space Telescope / Space Telescope Imaging Spectrograph. We find no strong emission or absorption features in the spectrum of X9. In particular, we place 3σ upper limits on the H α and He ii λ4686 emission line equivalent widths − EWH α ≲ 14 Å and |\rm -EW_He \small II \lesssim 9| Å, respectively. This is much lower than seen for typical X-ray binaries at a similar X-ray luminosity (which, for |L_{\rm 2--10 keV} ≈ 10³³--10³⁴| erg s−1 is typically − EWH α ∼ 50 Å). This supports our previous suggestion, by Bahramian et al., of an H-poor donor in X9. We perform timing analysis on archival far-ultraviolet, V- and I-band data to search for periodicities. In the optical bands, we recover the 7-d superorbital period initially discovered in X-rays, but we do not recover the orbital period. In the far-ultraviolet, we find evidence for a 27.2 min period (shorter than the 28.2 min period seen in X-rays). We find that either a neutron star or black hole could explain the observed properties of X9. We also perform binary evolution calculations, showing that the formation of an initial black hole/ He-star binary early in the life of a globular cluster could evolve into a present-day system such as X9 (should the compact object in this system indeed be a black hole) via mass-transfer driven by gravitational wave radiation.

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