An HI absorption distance to the black hole candidate X-ray binary MAXI J1535-571

Abstract

With the Australian Square Kilometre Array Pathfinder (ASKAP) we monitored the black hole candidate X-ray binary MAXI J1535--571 over seven epochs from 21 September to 2 October 2017. Using ASKAP observations, we studied the HI absorption spectrum from gas clouds along the line-of-sight and thereby constrained the distance to the source. The maximum negative radial velocities measured from the HI absorption spectra for MAXI J1535--571 and an extragalactic source in the same field of view are $-69\pm 4$ km s${}^{-1}$ and $-89\pm 4$ km s${}^{-1}$, respectively. This rules out the far kinematic distance ($9.3_{-0.6}^{+0.5}$ kpc), giving a most likely distance of $4.1_{-0.5}^{+0.6}$ kpc, with a strong upper limit of the tangent point at $6.7_{-0.2}^{+0.1}$ kpc. At our preferred distance, the peak unabsorbed luminosity of MAXI J1535--571 was $>78$ per cent of the Eddington luminosity, and shows that the soft-to-hard spectral state transition occurred at the very low luminosity of 1.2 -- 3.4 $\times$ 10${}^{-5}$ times the Eddington luminosity. Finally, this study highlights the capabilities of new wide-field radio telescopes to probe Galactic transient outbursts, by allowing us to observe both a target source and a background comparison source in a single telescope pointing.

Revised after favorable referee report from MNRAS Letters