On the prospects of imaging Sagittarius A∗ from space
Freek Roelofs (Radboud Universiteit Nijmegen)
Heino Falcke (Max-Planck-Institute for Radio Astronomy, Radboud Universiteit Nijmegen)
Christiaan Brinkerink (Radboud Universiteit Nijmegen)
Monika Moscibrodzka (Radboud Universiteit Nijmegen)
Leonid I. Gurvits (Joint Institute for VLBI ERIC, TU Delft - Astrodynamics & Space Missions)
Manuel Martin-Neira (European Space Agency (ESA))
Volodymyr Kudriashov (Radboud Universiteit Nijmegen)
Marc Klein-Wolt (Radboud Universiteit Nijmegen)
Remo Tilanus (Universiteit Leiden, Radboud Universiteit Nijmegen)
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Abstract
Very 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 μ as could be reconstructed, allowing for stronger tests of general relativity and accretion models than with ground-based VLBI.