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26 April 2024
 
  » arxiv » 2005.1339

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On the prospects of imaging Sagittarius A* from space
Freek Roelofs ; Heino Falcke ; Christiaan Brinkerink ; Monika Moscibrodzka ; Leonid I. Gurvits ; Manuel Martin-Neira ; Volodymyr Kudriashov ; Marc Klein-Wolt ; Remo Tilanus ; Michael Kramer ; Luciano Rezzolla ;
Date 4 May 2020
AbstractVery Long Baseline Interferometry (VLBI) at sub-millimeter waves has the potential to image the shadow of the black hole in the Galactic Center, Sagittarius A* (Sgr A*), and thereby test basic predictions of the theory of general relativity. We investigate the imaging prospects of a new Space VLBI mission concept. The setup consists of two satellites in polar or equatorial circular Medium-Earth Orbits with slightly different radii, resulting in a dense spiral-shaped uv-coverage with long baselines, allowing for extremely high-resolution and high-fidelity imaging of radio sources. We simulate observations of a general relativistic magnetohydrodynamics model of Sgr A* for this configuration with noise calculated from model system parameters. After gridding the $uv$-plane and averaging visibilities accumulated over multiple months of integration, images of Sgr A* with a resolution of up to 4 $mu$as could be reconstructed, allowing for stronger tests of general relativity and accretion models than with ground-based VLBI.
Source arXiv, 2005.1339
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