The 1.4 mm core of Centaurus A: First VLBI results with the South Pole Telescope

Abstract

Centaurus A (Cen A) is a bright radio source associated with the nearby galaxy NGC 5128 where high-resolution radio observations can probe the jet at scales of less than a light-day. The South Pole Telescope (SPT) and the Atacama Pathfinder Experiment (APEX) performed a single-baseline very-long-baseline interferometry (VLBI) observation of Cen A in January 2015 as part of VLBI receiver deployment for the SPT. We measure the correlated flux density of Cen A at a wavelength of 1.4 mm on a $\sim$7000 km (5 G$\lambda$) baseline. Ascribing this correlated flux density to the core, and with the use of a contemporaneous short-baseline flux density from a Submillimeter Array observation, we infer a core brightness temperature of $1.4\times 10^{11}$ K. This is close to the equipartition brightness temperature, where the magnetic and relativistic particle energy densities are equal. Under the assumption of a circular Gaussian core component, we derive an upper limit to the core size $\varphi =34.0\pm 1.8\mu \text{as}$, corresponding to 120 Schwarzschild radii for a black hole mass of $5.5\times 10^7{M}_{\odot }$.

arXiv comment9 pages, 5 figures, accepted for publication in ApJ

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• First VLBI detection of Fornax A
• Pointing Accuracy Improvements for the South Pole Telescope with Machine Learning