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First Space-VLBI Observations of Sagittarius A*

2021; IOP Publishing; Volume: 922; Issue: 2 Linguagem: Inglês

10.3847/2041-8213/ac3917

2041-8213

Michael D. Johnson, Y. Y. Kovalev, Mikhail Lisakov, P. A. Voitsik, C. R. Gwinn, G. Bruni,

Pulsars and Gravitational Waves Research

Abstract We report results from the first Earth-space VLBI observations of the Galactic Center supermassive black hole, Sgr A*. These observations used the space telescope Spektr-R of the RadioAstron project together with a global network of 20 ground telescopes, observing at a wavelength of 1.35 cm. Spektr-R provided baselines up to 3.9 times the diameter of the Earth, corresponding to an angular resolution of approximately 55 μ as and a spatial resolution of 5.5 R Sch at the source, where R Sch ≡ 2 GM / c 2 is the Schwarzschild radius of Sgr A*. Our short ground baseline measurements ( ≲ 80 M λ ) are consistent with an anisotropic Gaussian image, while our intermediate ground baseline measurements (100–250 M λ ) confirm the presence of persistent image substructure in Sgr A*. Both features are consistent with theoretical expectations for strong scattering in the ionized interstellar medium, which produces Gaussian scatter-broadening on short baselines and refractive substructure on long baselines. We do not detect interferometric fringes on any of the longer ground baselines or on any ground–space baselines. While space-VLBI offers a promising pathway to sharper angular resolution and the measurement of key gravitational signatures in black holes, such as their photon rings, our results demonstrate that space-VLBI studies of Sgr A* will require sensitive observations at submillimeter wavelengths.