NuSTAR observations of the Transient Galactic Black Hole Binary Candidate Swift J1858.6-0814: A New Sibling of V404 Cyg and V4641 Sgr?

Abstract

Swift J1858.6-0814 was discovered by Swift-BAT on October 25, 2018. Here we report on the first follow-up 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%$\pm 3$%, exhibiting a number of large flares throughout the observation. The hardness ratio (defined as $R_{10-79\mathrm{keV}}/R_{3-10\mathrm{keV}}$) of the flares tends to be soft, while the source spans a range of hardness ratios during non-flaring periods. The X-ray spectrum of the source shows strong reflection features, which become more narrow and peaked during the non-flaring 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 ($N_{\mathrm{H}}=1.4-4.2\times 10^{23}$ cm${}^{-2}$). This large intrinsic absorption is further supported by the energy spectra extracted from two flares observed simultaneously by NuSTAR and NICER. We find that the inner accretion disk of the source has a low inclination, $i<29^{\circ }$ ( 3$\sigma$ upper-limit), while the iron abundance in the disk is close to solar, $A_{\mathrm{Fe}}=1.0\pm 0.3$. We set a 90% confidence upper limit on the inner radius of the accretion disk of $r_{\mathrm{in}}<8r_{\mathrm{ISCO}}$, and, by fixing $r_{\mathrm{in}}$ to be at $r_{\mathrm{ISCO}}$, a 90% confidence lower-limit on the spin of the black hole of $a^{\ast }>0.0$. Lastly, 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.

arXiv commentAccepted for publication in the Astrophysical Journal

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• An Empirical Background Model for the NICER X-ray Timing Instrument
• The obscured X-ray binaries V404 Cyg, Cyg X-3, V4641 Sgr, and GRS 1915+105
• Observations of a radio-bright, X-ray obscured GRS 1915+105
• A persistent ultraviolet outflow from an accreting neutron star binary transient
• A NICER View of a Highly-Absorbed Flare in GRS 1915+105
• A shared accretion instability for black holes and neutron stars
• The INTEGRAL view on Black Hole X-ray Binaries
• The Changing-look Optical Wind of the Flaring X-ray Transient Swift J1858.6-0814
• Dips and eclipses in the X-ray binary Swift J1858.6-0814 observed with NICER
• The variable radio counterpart of Swift J1858.6-0814
• Soft X-ray emission lines in the X-ray binary Swift J1858.6-0814 observed with XMM-Newton-RGS: disc atmosphere or wind?
• Catalog of outbursts of neutron star LMXBs
• Long term radio monitoring of the neutron star X-ray binary Swift J1858.6-0814
• Phase resolved spectrum of the Crab pulsar from NICER
• X-ray Eclipse Mapping Constrains the Binary Inclination and Mass Ratio of Swift J1858.6-0814
• Detection of QPO Soft Lag during Outburst of Swift J1727.8-1613: Estimation of Instrinsic Parameters from Spectral Study
• A rapid optical and X-ray timing study of the neutron star X-ray binary Swift J1858.6-0814
• X-ray flashes from the low-mass X-ray binary IGR J17407-2808
• The Peculiar X-ray Transient Swift J0840.7-3516: an Unusual Low Mass X-ray Binary or a Tidal Disruption Event?
• The complex spectral behavior of the newly discovered neutron star X-ray binary Swift J1858.6-0814