Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry

TL;DR

This study measures the X-ray polarization of Cygnus X-1 to determine the accretion geometry, finding low polarization levels that suggest an extended or distant corona rather than a compact one near the black hole.

Contribution

First observational polarization measurement of Cygnus X-1's hard X-ray emission, constraining accretion geometry models in black-hole binaries.

Findings

Polarization fraction <8.6% at 90% confidence

Polarization angle aligned with jet axis

Indicates an extended or distant corona

Abstract

Black-hole binary (BHB) systems comprise a stellar-mass black hole and a closely orbiting companion star. Matter is transferred from the companion to the black hole, forming an accretion disk, corona and jet structures. The resulting release of gravitational energy leads to emission of X-rays. The radiation is affected by special/general relativistic effects, and can serve as a probe of the properties of the black hole and surrounding environment, if the accretion geometry is properly identified. Two competing models describe the disk-corona geometry for the hard spectral state of BHBs, based on spectral and timing measurements. Measuring the polarization of hard X-rays reflected from the disk allows the geometry to be determined. The extent of the corona differs between the two models, affecting the strength of relativistic effects (e.g., enhancement of polarization fraction and rotation of polarization angle). Here, we report observational results on linear polarization of hard X-ray (19-181 keV) emission from a BHB, Cygnus X-1, in the hard state. The low polarization fraction, <8.6% (upper limit at 90% confidence level), and the alignment of the polarization angle with the jet axis show that the dominant emission is not influenced by strong gravity. When considered together with existing spectral and timing data, our result reveals that the accretion corona is either an extended structure, or is located far from the black hole in the hard state of Cygnus X-1.