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On the prospects of imaging Sagittarius A* from space

Published online by Cambridge University Press:  07 April 2020

Freek Roelofs
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected]
Heino Falcke
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected] Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
Christiaan Brinkerink
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected]
Monika Moscibrodzka
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected]
Leonid I. Gurvits
Affiliation:
Joint Institute for VLBI ERIC, P.O. Box 2, 7990 AA Dwingeloo, The Netherlands Department of Astrodynamics and Space Missions, Delft University of Technology, 2629 HS Delft, The Netherlands
Manuel Martin-Neira
Affiliation:
European Space Research and Technology Centre (ESTEC), The European Space Agency, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
Volodymyr Kudriashov
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected]
Marc Klein-Wolt
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected]
Remo Tilanus
Affiliation:
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands email: [email protected] Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands
Michael Kramer
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
Luciano Rezzolla
Affiliation:
Institut für Theoretische Physik, Goethe-Universität, Max-von-Laue-Str. 1, 60438 Frankfurt, Germany
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Abstract

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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.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Bouman, K. L., Johnson, M. D., Dalca, A. V., et al. 2017, arXiv:1711.01357Google Scholar
Bower, G. C., Goss, W. M., Falcke, H., et al. 2006, ApJL, 648:L127L130CrossRefGoogle Scholar
Broderick, A. E., Fish, V. L., Johnson, M. D., et al. 2016, ApJ, 820:137CrossRefGoogle Scholar
Chael, A. A., Johnson, M. D., Narayan, R., et al. 2016, ApJ, 829:11CrossRefGoogle Scholar
Dexter, J., Agol, E., Fragile, P. C., & McKinney, J. C. 2010, ApJ, 717:10921104CrossRefGoogle Scholar
Falcke, H., Melia, F., & Agol, E. 2000, ApJL, 528:L13L16CrossRefGoogle Scholar
Ghez, A. M., Salim, S., Weinberg, N. N., et al. 2008, ApJ, 689:10441062CrossRefGoogle Scholar
Gillessen, S., Eisenhauer, F., Trippe, S., et al. 2009 ApJL, 692:10751109CrossRefGoogle Scholar
Goddi, C., Falcke, H., Kramer, M., et al. 2017, IJMPD, 26:1730001–239CrossRefGoogle Scholar
Gold, R., McKinney, J. C., Johnson, M. D., & Doeleman, S. S. 2017. ApJ, 837:180CrossRefGoogle Scholar
Johnson, M. D., Bouman, K. L., Blackburn, L., et al. 2017, ApJ, 850:172CrossRefGoogle Scholar
Johnson, M. D. & Gwinn, C. R. 2015. ApJ, 805:180CrossRefGoogle Scholar
Kudriashov, V. 2017. International Research Fellow Final Report, ESA-TECE-TN-007251Google Scholar
Lu, R.-S., Roelofs, F., Fish, V. L., et al. 2016, ApJ, 817:173CrossRefGoogle Scholar
Martin-Neira, M., Kudriashov, V., Barat, I., et al. 2017, In Proc. of the ARSI Workshop, ESTECGoogle Scholar
Mizuno, Y., Younsi, Z., Fromm, C. M., et al. 2018, ArXiv e-printsGoogle Scholar
Mościbrodzka, M., Falcke, H., Shiokawa, H., & Gammie, C. F. 2014, A&A, 570:A7Google Scholar
Mościbrodzka, M. & Gammie, C. F. 2018, MNRAS, 475:4354CrossRefGoogle Scholar
Psaltis, D., Özel, F., Chan, C.-K., & Marrone, D. P. 2015, ApJ, 814:115CrossRefGoogle Scholar
Roelofs, F., Falcke, H., Brinkerink, C., et al. 2019, A&A, 625:A124Google Scholar
Thompson, A. R., Moran, J. M., & Swenson, G. W., Jr. 2017, Interferometry and Synthesis in Radio Astronomy, 3rd EditionCrossRefGoogle Scholar