2019MNRAS.488L.129C

With the Australian Square Kilometre Array Pathfinder (ASKAP) we monitored the black hole candidate X-ray binary MAXI J1535-571 over seven epochs from 2017 September 21 to October 2. Using ASKAP observations, we studied the H I 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 H I absorption spectra for MAXI J1535-571 and an extragalactic source in the same field of view are -69 ± 4 and -89 ± 4 km s^–1, respectively. This rules out the far kinematic distance (9.3^+0.5_–0.6 kpc), giving a most likely distance of 4.1^+0.6_–0.5 kpc, with a strong upper limit of the tangent point at 6.7^+0.1_–0.2 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) x 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.