A decade of radio imaging the relativistic outflow in the peculiar X-ray binary Circinus X-1

TL;DR

This decade-long radio study of Circinus X-1 reveals relativistic jets with apparent velocities >= 12, variable morphology, and spectral changes, enhancing understanding of jet dynamics and accretion processes in this peculiar X-ray binary.

Contribution

The paper provides long-term radio imaging evidence of relativistic outflows and jet behavior in Circinus X-1, with detailed analysis of variability, spectral index, and polarization over ten years.

Findings

Relativistic jet apparent velocity >= 12

Detection of outbursts near orbital phases 0.0 and 0.5

Spectral index averaged -0.9, flatter during outbursts

Abstract

We present observations of the neutron star X-ray binary and relativistic jet source Circinus X-1 made at 4.8 and 8.6 GHz with the Australia Telescope Compact Array during a time interval of almost 10 years. The system shows significant variations in the morphology and brightness of the radio features on all timescales from days to years. Using the time delay between the successive brightening of the different components of the radio emission we were able to provide further evidence for the relativistic nature of the arcsec scale outflow, with an apparent velocity beta_app >= 12. No compelling evidence for an evolution of the orientation of the jet axis was found. We also place an upper limit on the proper motion of the system which is consistent with previous optical studies. Besides the previously reported radio flares close to the orbital phase 0.0 (interpreted as enhanced accretion at periastron passage), we also identified outbursts with similar properties near the orbital phase 0.5. The global spectral index revealed a preferentially steep spectrum over the entire period of monitoring with a mean value and standard deviation alpha=-0.9 +/- 0.6 (F_nu ~ nu^{alpha}), which became significantly flatter during the outbursts. Polarization was detected in one third of the epochs and in one case Faraday rotation close to the core of the system was measured.