NuSTAR Observations of the Transient Galactic Black Hole Binary Candidate Swift J1858.6-0814: A New Sibling of V404 Cyg and V4641 Sgr?
Hare J, Tomsick JA, Buisson DJK, Clavel M, Gandhi P, Garcia J, Grefenstette BW, Walton DJ, Xu Y (2020)
Publication Type: Journal article
Publication year: 2020
Journal
Book Volume: 890
Article Number: 57
Journal Issue: 1
Abstract
Swift J1858.6-0814 was discovered by the Burst Alert Telescope on Swift on 2018 October 25. Here we report on the first follow-up Nuclear Spectroscopic Telescope Array (NuSTAR) observation of the source, which shows variability spanning two orders of magnitude in count rate on timescales of ∼10-100 s. The power spectrum of the source does not show any quasi-periodic oscillations or periodicity, but has a large fractional rms amplitude of 147% ± 3%, exhibiting a number of large flares throughout the observation. The hardness ratio (defined as R 10-79keV/R 3-10keV) of the flares tends to be soft, while the source spans a range of hardness ratios during nonflaring periods. The X-ray spectrum of the source shows strong reflection features, which become more narrow and peaked during the nonflaring intervals. We fit an absorbed relativistic reflection model to the source spectra to place physical constraints on the system. Most notably, we find that the source exhibits a large and varying intrinsic absorbing column density (N H = (1.4-4.2) × 1023 cm-2). This large intrinsic absorption is further supported by the energy spectra extracted from two flares observed simultaneously by NuSTAR and the Neutron Star Interior Composition Explorer. We find that the inner accretion disk of the source has a low inclination, i < 29° (3σ upper limit), while the iron abundance in the disk is close to solar, A Fe = 1.0 ± 0.3. We set a 90% confidence upper limit on the inner radius of the accretion disk of r in < 8r ISCO and, by fixing r in to be at r ISCO, a 90% confidence lower limit on the spin of the black hole of a∗ > 0.0. Finally, we compare the properties of Swift J1858.6-0814 to those of V404 Cygni and V4641 Sgr, which both show rapid flaring and a strong and variable absorption.
Authors with CRIS profile
Involved external institutions
University of Southampton
United Kingdom (GB)
California Institute of Technology (Caltech)
United States (USA) (US)
University of California, Berkeley
United States (USA) (US)
University of Grenoble Alpes (UGA) / Université de Grenoble
France (FR)
University of Cambridge
United Kingdom (GB)
United Kingdom (GB)
California Institute of Technology (Caltech)
United States (USA) (US)
University of California, Berkeley
United States (USA) (US)
University of Grenoble Alpes (UGA) / Université de Grenoble
France (FR)
University of Cambridge
United Kingdom (GB)
How to cite
APA:
Hare, J., Tomsick, J.A., Buisson, D.J.K., Clavel, M., Gandhi, P., Garcia, J.,... Xu, Y. (2020). NuSTAR Observations of the Transient Galactic Black Hole Binary Candidate Swift J1858.6-0814: A New Sibling of V404 Cyg and V4641 Sgr? Astrophysical Journal, 890(1). https://dx.doi.org/10.3847/1538-4357/ab6a12
MLA:
Hare, Jeremy, et al. "NuSTAR Observations of the Transient Galactic Black Hole Binary Candidate Swift J1858.6-0814: A New Sibling of V404 Cyg and V4641 Sgr?" Astrophysical Journal 890.1 (2020).
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